The galaxy presents a generally smooth and elliptical morphology. There is a concentration of light towards the central region, suggesting a prominent bulge. The galaxy appears relatively undisturbed, showing no obvious signs of tidal tails or ongoing major mergers, although a possible minor disturbance cannot be ruled out. There is a slight elongation, giving it a somewhat cigar-like shape. The galaxy displays a color gradient, with the central bulge appearing more yellowish, possibly indicating an older stellar population, and the outer regions exhibit a slight bluer hue, suggesting the presence of younger stars or ongoing star formation. The overall structure indicates a relatively evolved system with a mix of stellar populations.
