The galaxy appears as an elliptical or lenticular type, displaying a smooth, relatively featureless morphology. It exhibits a concentrated, centrally-bright core that gradually diffuses outwards into a halo or bulge component. The overall shape is somewhat rounded, with no apparent spiral arm structures or significant distortions indicative of recent major merger events. There is potentially a minor, localized asymmetry that may indicate minor disturbance of a merging partner but it is not clear. The galaxy exhibits colors that are characteristic of an older stellar population; redder in appearance. This suggests that it is dominated by evolved stars, with a relatively low ongoing star formation rate.
