The galaxy presents a generally elliptical morphology, exhibiting a concentrated central bulge region that dominates its overall luminosity. A faint, diffuse halo surrounds the central region, exhibiting a gradual decline in surface brightness with increasing radial distance. Color gradients are apparent across the galaxy, with the central bulge showing bluer coloration, potentially indicating the presence of younger stellar populations. Conversely, the outer regions of the galaxy halo show a more pronounced yellow hue, suggestive of older, redder stars. There is some evidence of disrupted symmetry in the halo, hinting at possible tidal interactions or recent merger events. The overall structural integrity of the galaxy appears relatively intact, though the subtle asymmetries merit further investigation.
