The galaxy presents as a yellowish, elliptical morphology. It exhibits a centrally concentrated luminosity profile, with a smooth, diffuse halo extending outwards. There is little evidence of spiral arm structure or significant dust lanes. The galaxy appears to be relatively isolated, with no obvious tidal features or nearby companion galaxies suggesting recent or ongoing merger activity, although a slight disturbance cannot be ruled out. The overall color suggests a relatively evolved stellar population, potentially dominated by older, redder stars. Star formation may be present, but at a relatively low level.
