The galaxy presents as a relatively smooth, centrally concentrated object. It has a somewhat elliptical morphology, appearing more "in between" round and cigar shaped, rather than distinctly circular. There is a bright central bulge, possibly indicative of an older stellar population. Faint, diffuse spiral arm structures may exist in the outer regions, but this is uncertain, and if present, they show minimal signs of ongoing star formation. The galaxy's color appears to be largely yellow-red, suggesting a population dominated by older, redder stars. There are no strong indications of any major disturbances or mergers. Small signs of minor disturbances may be present. Overall, the galaxy seems to be relatively quiescent.
