The galaxy exhibits a complex morphology suggestive of an ongoing or recent merger event. The main body of the galaxy appears relatively smooth, but it is surrounded by several distinct, brighter knots of light. The overall shape deviates significantly from a regular elliptical or spiral form; it appears amorphous and disturbed.

Color variations are present within the galaxy. The central region displays a yellowish-white hue, indicative of a population of older stars. Surrounding this core, there are regions with a reddish tint, which could signify areas of active star formation obscured by dust, or simply a population of cooler, older stars. There are also areas tinged with green.

Given the irregular shape and color variations, this galaxy is likely undergoing significant gravitational interactions. These interactions could be triggering bursts of star formation or disrupting the existing stellar distribution. Further spectroscopic analysis would be valuable in determining the stellar populations, redshift, and presence of any active galactic nucleus.
