The galaxy presents as a relatively compact, elongated structure, suggestive of a disk galaxy viewed at a significant inclination. The central region exhibits a concentrated luminosity, likely indicative of a prominent galactic bulge. The light distribution appears smoother than that of a spiral galaxy, possibly indicating a lack of well-defined spiral arms or the arms being tightly wound. Overall, the galaxy is smooth in appearance. There appears to be little to no disturbance or recent merging event.
