This galaxy exhibits an elliptical morphology, appearing largely smooth with a highly concentrated central bulge. Its color profile indicates a redder population, with older stars dominating the light output. The galaxy appears to be generally undisturbed with no clear signs of recent major mergers, though the presence of some diffuse light around the main body could suggest a past interaction or ongoing minor disturbance. The overall shape is predominantly round, with only a slight deviation towards an elongated form.
