The galaxy presents as a relatively compact object with a smooth, centralized light distribution, suggesting it is likely an elliptical or lenticular galaxy. The galaxy has a generally round morphology, exhibiting a noticeable lack of spiral arm structures. There's a suggestion of a possible minor disturbance within the galactic structure, potentially indicative of a past or ongoing minor merger event or internal dynamics. The core of the galaxy seems to be brighter than the outer edges, potentially implying a higher density of stars towards the center. Its overall color indices suggest it is not strongly actively star-forming.
