The galaxy appears to be a relatively compact object, exhibiting a somewhat elliptical morphology. There is a smooth, centrally concentrated light distribution suggesting a spheroid-dominated structure. However, there appears to be some asymmetric light distribution, possibly a faint tidal tail or stellar stream extending from the main body, hinting at a past or ongoing interaction. The color gradient indicates a redder core region which implies an older stellar population, while the outer regions are slightly bluer, suggesting the presence of younger stars. The presence of disturbances or merging cannot be completely ruled out. Overall, the galaxy appears to be an elliptical galaxy with possible signs of interaction or recent merger activity.
