This galaxy presents as a primarily smooth, elliptical morphology, with a concentrated central bulge. The core exhibits a bright, relatively uniform luminosity profile, suggestive of an older stellar population. The isophotes appear generally regular, though subtle irregularities along the outer edges hint at possible tidal interactions or minor disturbances. The galaxy displays a slight color gradient, transitioning from a bluer hue in the central regions to redder tones in the outer halo. There appears to be a subtle, slightly disturbed, disk structure. Overall, the galaxy demonstrates characteristics of a relatively evolved system, potentially undergoing minor morphological changes due to past mergers or interactions.
