The galaxy presents a largely smooth morphology, with a concentrated central bulge that dominates the overall light profile. The elliptical shape is near-spherical. There's little evidence of spiral arms or significant disk-like structures. Color gradients are observed, with the central region appearing yellowish, potentially indicative of an older stellar population. The outer regions exhibit a subtle bluer hue suggesting the presence of some younger stars. No apparent major mergers or tidal disturbances are noted, although there may be a very slight asymmetry in the outer regions. Overall, the galaxy appears to be a relatively quiescent system.
