The galaxy presents as a relatively smooth, elliptical or lenticular structure. Its light distribution appears concentrated toward the center, with a bright, yellowish core indicative of an older stellar population. The galaxy exhibits a spheroidal shape, with only a slight deviation from perfect circularity. There's no obvious presence of spiral arms or dust lanes, suggesting a lack of significant ongoing star formation. The outer regions of the galaxy appear fainter and bluer, possibly indicating a small amount of younger stars. Overall, the galaxy appears to be a relaxed, evolved system.
