The galaxy appears to be an elliptical or lenticular type, exhibiting a generally smooth, featureless morphology with a bright, concentrated central bulge. The overall shape is neither perfectly spherical nor highly elongated, appearing somewhere in between. There is no clear spiral arm structure visible. A faint disk may be present, though it is not well defined. There is some suggestion of minor disturbances in the outer regions, hinting at a possible past interaction. The color distribution indicates a predominantly older stellar population, particularly within the bulge, which exhibits a yellowish-white hue. The outer regions of the disk (if present) show a slightly bluer tint, suggesting the possibility of some ongoing star formation.
