The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a bright, concentrated core, decreasing in luminosity outwards. The galaxy's color profile suggests a population of older stars, appearing more red in the image. There is no clear evidence of spiral arms or significant dust lanes. The overall shape tends to be round. There may be a minor disturbance or tidal feature in the outer regions, but it's not pronounced, with no obvious signs of a recent major merger. The galaxy likely possesses a substantial stellar mass and displays moderate star formation activity.
