The galaxy presents as a concentrated, ellipsoidal light distribution, suggesting a predominantly spheroidal morphology. A significant fraction of the galaxy's light is concentrated in the central region, indicative of a prominent galactic bulge. The galaxy's color is generally yellowish-orange, suggesting an older stellar population with a lower rate of star formation. The overall structure appears relatively undisturbed, with no obvious signs of ongoing major mergers or tidal interactions. There might be a faint, disk-like component around the bulge. Overall, the galaxy has characteristics of a massive system with a significant population of evolved stars.
