The galaxy presents a complex morphology, appearing to be in a state of interaction or recent merger. The primary body of the galaxy exhibits a smooth, elliptical profile, suggesting a significant spheroidal component. A distinct, bright, and slightly bluer region is observed in the center of the galaxy, hinting at a possible active galactic nucleus or a region of intense star formation. 

There is a faint tail of material extending from the main galactic body. The galaxy displays a general distribution of light across the visual spectrum. The lack of distinct spiral arms or prominent dust lanes supports the classification of a relatively featureless system, likely an elliptical galaxy or early-type spiral galaxy. The overall shape is generally rounded but with visible asymmetries due to potential interactions.
