The galaxy presents a somewhat elongated, cigar-shaped morphology. It exhibits a concentrated central bulge region, characterized by a yellowish-orange hue, suggesting an older stellar population. The outer regions of the galaxy appear fainter and more diffuse. There is a slight suggestion of faint disk-like structure or perhaps a tidal tail extending from one end of the galaxy. The overall structure appears relatively undisturbed, with no obvious signs of major mergers or strong gravitational interactions. The galaxy is likely an early-type spiral or elliptical galaxy with little current star formation.
