The galaxy exhibits a largely smooth morphology, indicative of an elliptical or lenticular type. There is a prominent, centrally concentrated bulge region displaying a reddish hue, which may suggest an older stellar population. Surrounding the core is a more diffuse halo with a bluish tinge, possibly indicating some presence of younger, hotter stars or ongoing star formation activity, albeit at a relatively low level. The overall shape appears close to elliptical, with no clear signs of a distinct disk or spiral arms. There is no apparent visual evidence of tidal disturbances or major mergers.
