The galaxy presents as a largely smooth, elliptical morphology, characterized by a concentrated central bulge. It exhibits a luminosity profile that gradually decreases from a bright core to a fainter, diffuse halo. The galaxy appears to be generally elongated in shape, with a major axis approximately five times the minor axis. There are no prominent spiral arm structures or dust lanes visible. Overall, the galaxy presents a largely undisturbed appearance, with no signs of a recent or ongoing major merger event. The light from the galaxy has a red-yellow hue, which may be indicative of an older stellar population. The color suggests minimal ongoing star formation activity.
