The galaxy presents an elliptical morphology when viewed from our perspective. It exhibits a concentrated central bulge that is bright and yellowish, suggesting a population of older stars. Fainter, bluer regions extend outwards from the bulge, forming what appears to be a disk. This disk seems to be tilted with respect to our line of sight, giving the galaxy an elongated appearance. There is evidence of some dust obscuration within the disk, particularly along the near side, that contributes to the galaxy's overall color. No distinct spiral arms are visible. The outer regions of the galaxy fade gradually into the background, with a relatively smooth transition. There is no evidence of any major mergers or significant tidal disturbances.
