The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge with a gradual fade in luminosity towards its periphery. There are no apparent spiral arms or significant dust lanes visible. The color profile appears relatively uniform across the galaxy, with a slightly yellowish hue dominating the central region, suggesting a population of older stars. There is a lack of significant blue light, which would indicate the presence of younger, hotter stars formed in recent starburst events. Overall, the galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. It possesses a round appearance with no cigar-shaped appendages. Subtle hints of disturbances may be present in the faint outskirts, but these are not prominent.
