The galaxy presents as a generally smooth, elliptical-like structure. It exhibits a concentrated central bulge with a gradual decrease in luminosity extending outwards. There is a slight elongation observed, with the overall shape leaning towards a more cigar-shaped morphology. There are no readily apparent spiral arms or distinct dust lanes visible in the image, suggesting the galaxy may be an early-type, relatively quiescent system with minimal recent star formation. There is a small hint of a faint disk. There are no clear signs of major disturbances or ongoing mergers, although a slight asymmetry hints towards a possible minor gravitational interaction in its past.
