The galaxy presents an overall elliptical morphology, though some features suggest a possible disk component. It has a centrally concentrated bulge region that appears yellowish-white, indicative of an older stellar population. The outer regions exhibit a bluer hue, suggestive of more recent star formation activity. The galaxy's overall shape is more elongated than circular; a mild cigar shape. There is no evidence of major mergers or significant tidal disturbances. The galaxy is not perfectly smooth; some patchiness indicates substructure and possibly faint spiral arms.
