The galaxy presents as a single, relatively smooth object. Its overall shape is elliptical, appearing elongated, with an aspect ratio suggesting a classification between E4 and E6 on the Hubble sequence. A concentrated central bulge exhibiting a warmer, redder color profile is observed, potentially indicative of an older stellar population. Surrounding the central bulge is a fainter, diffuse halo with bluer hues. There is no evidence of spiral arms, prominent dust lanes, or ongoing major mergers. Subtle asymmetric features suggest a potential minor interaction. The lack of easily discernible star-forming regions implies a low star formation rate. Overall, it appears to be a galaxy with evolved stellar populations and minimal recent star formation.
