The galaxy presents as a centrally concentrated object with a generally smooth appearance, although some slight irregularities can be observed. It appears to be somewhat elliptical in shape, trending towards a more rounded morphology, with the absence of a clear disk structure. The galaxy exhibits a color gradient, transitioning from a bright, yellowish central region to a more diffuse, reddish-tinged outer halo. The core is significantly brighter than the surrounding regions, suggesting a higher density of stars and/or an active galactic nucleus. There are no obvious signs of major mergers or tidal disturbances affecting its structure, although subtle asymmetries may indicate minor interactions in its past. The relatively red color suggests a population of older stars and possibly suppressed star formation.
