The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, appearing almost spherical. A faint, diffuse halo surrounds the core, gradually fading into the background. There is minimal evidence of spiral arms or prominent dust lanes within the resolution of this image. The light distribution appears to be largely uniform across the galaxy, with a colour gradient suggesting older stellar populations dominate. There are no indications of major mergers or significant tidal disturbances affecting the galaxy's morphology.
