The galaxy presents as a relatively smooth, elliptical object with a concentrated central bulge. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. Moving outwards from the core, the galaxy displays a diffuse, reddish halo, indicative of a decrease in stellar density and potentially a greater proportion of evolved, cooler stars. The overall shape is close to circular but slightly elongated along one axis. No distinct spiral arm structures or dust lanes are readily apparent in this image. There is a lack of blue light, signifying that star formation is likely not dominant in the region. The light distribution appears to follow a Sersic profile, with a gradual decrease in brightness moving away from the center, indicative of an older stellar population.
