The galaxy presents as a disturbed system, with a complex morphology indicative of a possible ongoing or recent merger event. There are asymmetric features and distorted structures that cannot be easily characterized by a simple elliptical or spiral classification.

The primary body of the galaxy appears somewhat diffuse, with a slightly brighter central region. There is a suggestion of tidal features extending from the main galactic body, which could be tidal tails or bridges produced by gravitational interactions. These structures are faint and elongated, contributing to the overall disturbed appearance.

The color distribution across the galaxy suggests variations in stellar populations. Bluer regions are present, potentially indicating areas of active star formation, while yellower or redder regions may contain older stellar populations. Patches of varying color are visible, contributing to the overall mottled and irregular appearance of the galaxy. A significant portion of the galaxy is generally blue-green in color.

Based on the morphological irregularities and color variations, it seems likely that this galaxy has experienced significant gravitational interactions or a recent merger event, which has disrupted its original structure and triggered bursts of star formation in certain regions. 
