The galaxy appears as a relatively compact, centrally concentrated object. Its overall morphology seems to be largely smooth with a subtle, diffuse halo. The object’s shape is generally in between round and elliptical, with only a slight elongation. Some minor disturbances may be present, as suggested by the slight asymmetry in the outer regions. There isn't any prominent spiral arm structure, and the galaxy is likely a relatively quiescent system. The galaxy's color indices suggest a stellar population that is dominated by older, redder stars, which is consistent with a low star formation rate.
