The galaxy presents as a centrally concentrated object exhibiting a relatively smooth morphology. The dominant feature is a bright, spheroidal core that transitions gradually into a more diffuse halo. The color profile suggests a population of older stars, with a redder hue dominating the central bulge. There is a faint hint of a disk structure surrounding the bulge, characterized by a bluer color, potentially indicative of ongoing, albeit mild, star formation within the disk. No prominent spiral arms or bar structures are readily apparent. There is a very slight irregularity in the morphology suggestive of a minor gravitational interaction or past merger event, but it does not dominate the overall structure. Overall, this galaxy appears to be a massive, relatively evolved system, potentially a lenticular or early-type spiral galaxy viewed at a distance.
