The galaxy presents as a relatively smooth, centrally concentrated object. There's a noticeable radial gradient in luminosity, with the core region appearing significantly brighter than the outer regions. The overall morphology appears elliptical, with no clear evidence of spiral arms or a distinct disk structure. The color profile suggests a moderate stellar population, potentially skewed towards older stars, based on the yellowish hue. There's no indication of active galactic nuclei activity or significant dust lanes obscuring the central regions. The galaxy's light is fairly regular and undisturbed, with no signs of major mergers or tidal tails.
