The galaxy presents as a generally smooth, elliptical-like structure. It exhibits a concentrated central bulge that graduates outwards into an extended, less dense halo. The color profile suggests an older stellar population, with a yellowish-red hue dominating the central region, indicating the presence of evolved stars. There are no prominent spiral arms or dust lanes visible. The galaxy appears relatively undisturbed, without any significant signs of tidal interactions or ongoing major mergers. The shape is more "in-between" round and cigar shaped, slightly elongated. There is evidence of a low star formation rate.
