The galaxy appears to be relatively smooth in structure, with a centrally concentrated brightness profile. It exhibits a generally elliptical shape, displaying a slight elongation. The color profile suggests a population of older stars, with a redder overall hue. There is some suggestion of minor disturbances or interactions, evidenced by a faint, extended feature that extends from the main body of the galaxy. Overall, it presents characteristics that would classify it as a relatively massive galaxy, showing subdued star formation activity.
