The galaxy presents as a roughly elliptical structure, exhibiting a smooth overall morphology. A bright, concentrated central bulge dominates the galaxy's luminosity profile. The surrounding disk appears relatively featureless with some faint, diffuse spiral arm structures possibly present, though poorly defined. The color gradient suggests a population of older stars in the central regions, with a possible hint of bluer, younger stars in the outer regions. There is no obvious evidence of strong tidal interactions or a major merger event, although some minor disturbances cannot be ruled out based on this image alone. The galaxy does appear generally undisturbed and relatively isolated.
