The galaxy presents as a spiral type, however, its features appear somewhat disturbed. It displays a central, moderately bright bulge region that exhibits a yellowish hue. This suggests a population of older stars. Fainter, bluer regions can be seen extending outward, hinting at ongoing, but relatively low, star formation in the disk. Overall, the galaxy exhibits a moderately smooth morphology, without a strong presence of spiral arm structure. There is evidence of a minor disturbance visible within the galaxy's structure, possibly the result of a past interaction. The galaxy is roughly elliptical in shape, though not highly elongated.
