The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that fades into a more diffuse halo. The color profile suggests an aging stellar population, with a redder hue concentrated toward the core becoming slightly bluer in the outer regions. There's no clear evidence of prominent spiral arms or significant dust lanes. The overall shape appears slightly elongated. There is no clear indication of ongoing major merger activity, though subtle disturbances in the outer halo cannot be ruled out. The galaxy exhibits substantial luminosity, indicative of a relatively high stellar mass and moderate star formation activity.
