The galaxy presents as a largely smooth, elliptical morphology, with a concentrated central bulge and a radial decrease in luminosity. The color gradient suggests an older stellar population dominating the core, exhibiting a yellowish-orange hue. There appears to be a subtle, surrounding halo with slightly bluer tones, potentially indicating the presence of a younger stellar population in the outer regions, though this is less pronounced. The overall structure shows little evidence of spiral arms or significant disk-like features. There are no indications of ongoing major mergers or tidal disturbances, although subtle asymmetries may suggest minor interactions in its past. The galaxy's shape is generally round, exhibiting minimal elongation.
