The galaxy presents an overall smooth appearance with a centrally concentrated bulge. The light distribution appears to be relatively uniform with no obvious spiral arms or distinct features. The galaxy exhibits a slight ellipticity, appearing somewhat elongated rather than perfectly spherical. The color profile suggests a redder hue towards the center, possibly indicating an older stellar population, and a bluer hue extending outwards, suggesting younger stars. There are some slight disturbances in the structure, though it is hard to determine if they are internal or external.
