The galaxy presents as a single, relatively smooth object with a concentrated central region. It exhibits a nearly elliptical morphology, deviating slightly from perfect circularity. The galaxy's color profile suggests a predominantly older stellar population, indicated by the yellowish-red hue concentrated in the central bulge, likely dominated by evolved stars. There is no clear evidence of significant dust lanes or spiral arm structures. The galaxy displays no prominent tidal features, plumes, or other signs of recent major mergers, although minor disturbances cannot be ruled out. The overall impression is that of a relatively quiescent galaxy, potentially an early-type galaxy or a spiral galaxy with a dominant bulge and tightly wound arms that are not easily resolvable at this scale.
