The galaxy presents as a generally smooth, elliptical-shaped structure. It exhibits a concentrated central bulge that emits strongly in the yellow-orange wavelengths, suggesting a population dominated by older stars. Moving outward from the center, the light gradually fades, with a diffuse halo. There is a very slight suggestion of a disk component, though not well defined. There is no evidence of spiral arms or significant dust lanes, nor are there any obvious signs of ongoing major mergers or tidal disturbances. The overall morphology indicates a relatively evolved system.
