The galaxy presents a generally elliptical morphology, appearing largely smooth in texture, with a concentrated central bulge exhibiting a yellow-orange hue. The color suggests a dominant population of older stars. Extending outwards from the central region, there is a more diffuse halo. Evidence of disk-like structures or prominent spiral arms is not apparent, but there may be some minor disturbances or subtle features within the outer regions. The galaxy does not appear to be undergoing a major merger, though there could be some minor tidal interactions or recent accretion events as evidenced by the slightly disturbed outer isophotes. The overall appearance suggests a relatively evolved system, likely characterized by lower specific star formation rate. The approximate physical diameter is 7.76 kpc.