The galaxy presents a generally smooth, elliptical morphology with a slight elongation. Its core exhibits a concentrated, bright, and somewhat reddish-yellow hue, indicative of an older stellar population. The surrounding halo gradually diffuses outward from the center, displaying a bluer color gradient, possibly suggesting the presence of younger stars. There are no apparent spiral arm structures or significant dust lanes visible within the image. The overall structure is relatively undisturbed, with no readily observable signs of recent major mergers or tidal disruptions. The galaxy's apparent size is moderately small, and it appears to be a fairly compact system.
