The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge that gradually fades into the outer regions, with a generally round morphology. There is a noticeable lack of distinct spiral arms or prominent dust lanes. The color profile suggests a population of older stars, as indicated by its redder hue. There is no visual evidence of a major merger or significant tidal disturbances, it does not show signs of active star formation. The galaxy appears to be a relatively isolated system in its current state.
