The galaxy appears to be a relatively smooth, centrally concentrated object. Its overall shape is elliptical, trending towards a more spherical morphology. The galaxy exhibits a radial gradient in color, appearing reddish in the center and fading towards the outer edges. The core is bright and concentrated and smoothly transitions to the outer regions. There is evidence of some minor disturbances or irregularities in the surrounding light distribution, possibly indicating interactions or past mergers with smaller satellite galaxies. Faint, diffuse features may hint at tidal tails or debris fields. There is also some indication of a disk component.
