The galaxy presents a largely smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, indicating a bulge-dominated system. There's a noticeable lack of well-defined spiral arms or distinct features characteristic of disk galaxies. The galaxy appears somewhat rounded in shape, with a slight deviation from perfect circularity. Faint, diffuse extensions are observed, suggestive of possible tidal interactions or a halo of stellar material. The color gradient implies a population of older stars, consistent with its passive star formation rate and substantial stellar mass. Evidence of recent major merging events is not obvious. The central region is the brightest, with the light fading outwards in a smooth manner.
