This galaxy presents as a primarily smooth object, exhibiting an elliptical morphology. The central region displays a notable concentration of older stars, evidenced by its reddish-yellow hue. The outer regions exhibit a bluer tint, suggesting the presence of younger stars. The galaxy appears to be in a relatively isolated state, with no clear indication of major disturbances or ongoing mergers. There is a mild asymmetry observed in the morphology, with one side appearing slightly more extended or disturbed than the other. This could possibly indicate an interaction in the past. The overall structure shows an elongated shape, leaning towards being cigar shaped. Star formation rates appear to be low, and the galaxy appears to be very massive.
