The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that dominates the overall light profile, surrounded by a less luminous and more diffuse halo. The color appears yellowish-white, suggesting a stellar population dominated by older, less massive stars. There is no obvious evidence of spiral arm structure or significant dust lanes. The galaxy appears relatively undisturbed, without any clear signs of ongoing mergers or tidal interactions. There may be a subtle flattening of the isophotes indicating a possible elongated shape, but the deviation from perfect circularity is not significant.
