The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, with a gradual decrease in brightness outward from the core. The shape approximates a prolate spheroid, elongated along its major axis. There is a subtle color gradient, with the central region appearing slightly more yellow-white, suggesting an older stellar population. No distinct spiral arms or prominent dust lanes are discernible within the resolution limits. The overall structure appears largely undisturbed, with no obvious signs of recent major mergers or tidal interactions. A faint, diffuse halo may be present, extending beyond the brighter central region.
