The galaxy presents a generally smooth, elliptical morphology. The light distribution appears concentrated towards the center, indicating a prominent bulge. There is little evidence of significant spiral arm structure or dust lanes. The galaxy exhibits a color gradient, with the central region appearing more yellow/red, possibly indicating an older stellar population, while the outer regions are slightly bluer, hinting at the presence of some younger stars or ongoing star formation. The galaxy appears relatively isolated, showing no obvious signs of recent major mergers or tidal disturbances. There are faint features or minor disturbances that may indicate a prior interaction or minor merger event. The roundness of the galaxy suggests it is likely an E0-E3 elliptical type, possibly closer to E0.