The galaxy presents as a relatively smooth, elliptical or lenticular structure. There is a notable concentration of light towards the galactic center, suggesting a prominent bulge. The color profile indicates a population of older stars, inferred from the reddish-yellow hue observed, though some bluer regions may be sparsely present. The galaxy displays a moderate degree of roundness, deviating slightly from a perfect circular shape. There's no apparent evidence of major disturbances, tidal tails, or ongoing mergers. Star formation appears to be occurring but at a low rate.
