The galaxy presents as a somewhat elliptical structure. It exhibits a concentrated central bulge region that appears bright and yellowish-white in color, suggesting a population of older stars. The overall form appears relatively smooth, showing little evidence of spiral arms or significant dust lanes. The outer regions of the galaxy show hints of a bluer color. There is no obvious evidence of a major ongoing merger or tidal disruption. The galaxy's shape indicates a morphology somewhere between a sphere and a cigar, with a preference towards a more spheroidal appearance. There might be minor disturbances in the outer regions of the galaxy.
