The galaxy presents as a relatively smooth, centrally concentrated object, likely an elliptical galaxy given the lack of discernible spiral arm structure. It appears primarily spheroid in shape, though a slight elongation is noticeable, suggesting a deviation from perfect roundness. The light distribution is concentrated towards the center, with a diffuse halo that gradually fades into the background sky. There are no obvious signs of ongoing major mergers or tidal disturbances, however there may be evidence of some slight minor disturbance. The galaxy's core is characterized by a bright, somewhat blue-ish hue, indicating a potential presence of younger stellar populations or active galactic nucleus activity, although the overall color suggests a population of older stars.
