The galaxy appears to be an elliptical galaxy with a smooth, spheroidal morphology. It exhibits a relatively concentrated central bulge, characterized by a bright, diffuse glow, suggesting a significant population of older stars. There is minimal evidence of spiral arm structure or significant dust lanes within the visible spectrum. The overall color profile indicates a predominantly red-shifted population suggesting low ongoing star formation activity. There's slight indication of minor disturbances. The shape is mostly round, but slightly in between round and cigar shaped.
