The galaxy presents a primarily smooth, elliptical morphology. There is a concentrated central bulge exhibiting a yellowish hue, suggesting a population of older stars. The outer regions of the galaxy display a bluer tint, hinting at the presence of some younger stars. Although largely smooth, there may be a faint hint of a disk or spiral arms, but the overall appearance is dominated by the spheroidal component. There is no significant evidence of ongoing major mergers or tidal disturbances affecting the overall structure. The galaxy appears relatively isolated and undisturbed.
