The galaxy presents a predominantly elliptical morphology. A smooth, concentrated bulge dominates the central region, exhibiting a yellow-orange hue, suggestive of an older stellar population. The outer regions show a more diffuse and less structured distribution of light, with a color gradient indicating progressively bluer colors towards the periphery. There is a slight asymmetry in the outer regions, but no obvious signs of spiral arm structure. No strong tidal features or distortions are apparent, which could indicate a recent major merger event. The galaxy appears relatively isolated.
