The galaxy presents as an elliptical morphology, appearing largely smooth and spheroidal in shape, lacking prominent spiral arms or a distinct disk-like structure. It exhibits a concentrated central bulge that gradually fades into the outer regions. The galaxy displays a yellowish-red hue, suggesting a dominant population of older stars and a low rate of ongoing star formation. There is no clear evidence of significant dust lanes or tidal features, and the galaxy appears relatively undisturbed. The galaxy appears to be relatively isolated, with no obvious signs of ongoing or recent merger activity. The overall luminosity profile seems regular and symmetric.
