The galaxy appears to be an elliptical galaxy with a smooth, fairly symmetrical structure. Its color profile suggests a population dominated by older stars, likely of a redder or yellower hue, particularly concentrated toward the galaxy's core. There is no visible indication of spiral arms or a significant disk component. The galaxy exhibits a slightly elongated shape, leaning toward round, with no apparent signs of a major ongoing merger or significant tidal disturbance. The general morphology suggests a relatively quiescent state, without intense star formation activity.