The galaxy presents as a concentrated central bulge, surrounded by a fainter, more diffuse halo. The shape is generally elliptical, tending toward a spheroidal morphology, with a slight elongation. The light distribution is relatively smooth, with no obvious spiral arm structures or dust lanes visible. There is no pronounced central point-source indicative of a strong active galactic nucleus. The color appears overall to be moderately red, suggesting a population of older, evolved stars, with the possible presence of some intermediate-age stars as well. There is no visual evidence of ongoing major mergers or significant tidal disturbances.
