This galaxy exhibits a mixed morphology, appearing primarily smooth but with subtle features indicative of a past or ongoing interaction. The galaxy's core presents a bright, concentrated region, suggestive of an older stellar population, potentially an elliptical component. Extending outwards, a fainter, more diffuse halo is visible. This halo shows asymmetry and a slightly irregular shape, hinting at possible tidal disturbances. A secondary, less luminous region is connected to the primary body, either through the merging of a smaller galaxy or through an extended tidal tail. The color gradient observed suggests some ongoing star formation, but at a relatively low rate overall, and is likely located primarily in the slightly bluer area that might be a merging galaxy. The lack of clearly defined spiral arms or a prominent disk structure reinforces the classification as an object transitioning between elliptical and interacting systems.
