The galaxy presents as a somewhat elongated, smooth structure, suggestive of an elliptical morphology. It has a bright central bulge or core, surrounded by a fainter, more diffuse halo. The galaxy exhibits a color gradient, appearing more yellow/white in the central regions, possibly indicating an older stellar population, with a subtle shift toward blue in the outer regions, indicative of the presence of younger stars. There is no prominent dust lane or spiral arm structure visible. The overall appearance suggests that the galaxy is relatively undisturbed, and does not appear to be undergoing a major merging event, although subtle signs of past interaction cannot be fully ruled out.
