The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a generally rounded shape, with a slight elongation not strongly deviating from circularity. The light distribution appears centrally concentrated, with a gradual decrease in luminosity moving outwards from the center. There is no apparent disk structure. The galaxy displays a fairly uniform color, suggesting a lack of ongoing, significant star formation. The overall color is a muted blueish-white, indicating that the stellar population is primarily composed of older stars. There are no obvious signs of interaction or recent mergers, although there may be very minor disturbances, these are not significant. 
