The galaxy presents as a generally smooth, elliptical-like structure with a concentrated central bulge. The galaxy exhibits a predominantly yellow-red hue, suggesting an older stellar population and a relatively low rate of ongoing star formation. There is minimal evidence of spiral arm structure or significant disk features. The observed roundness indicates a low degree of ellipticity, tending toward a spherical shape. Indications of merger activity are minor to non-existent based on the smooth features of this galaxy, with no obvious signs of tidal tails or distortions. The galaxy exhibits a concentrated brightness profile.
