The galaxy presents a generally smooth and rounded morphology. The primary light concentration exhibits a centrally condensed core that fades into a diffuse halo. Some slight evidence of a disc-like structure appears through subtle variations in the light distribution. Indications of a potential minor disturbance are present in the form of a faint, irregular extension or tidal feature, or a possible minor galaxy merger. This galaxy is of intermediate size, and has colors that appear to be in the blue-green range in the inner parts of the galaxy, which may be indicative of active star formation. Overall, this galaxy appears relatively evolved and quiescent, as the light is dominated by older stellar populations, yet there is evidence to support that some star formation is occurring.
