The galaxy presents as a somewhat elliptical structure with a smooth, concentrated central bulge. The galaxy exhibits a yellowish-orange color profile suggesting a relatively older stellar population with a low star formation rate. There are no prominent spiral arms or strong dust lanes visible. The overall structure appears undisturbed, with no obvious signs of ongoing major mergers or tidal distortions. The apparent lack of substructure and the dominant smooth component indicate that it may be an early-type galaxy.
