The galaxy presents as a largely featureless, elliptical-like structure with a concentrated central bulge. Its color profile indicates a dominant population of older stars, exhibiting a yellowish-orange hue, consistent with a lack of significant ongoing star formation. There is no discernible spiral arm structure or prominent dust lanes visible. The galaxy appears relatively isolated, with no obvious signs of tidal interactions or nearby companion galaxies. Its morphology suggests a quiescent system that is likely a high mass system with a relatively low specific star formation rate. The overall smooth appearance indicates that it is round.
