The galaxy presents as a spiral galaxy, viewed at a moderate inclination. The galactic bulge appears moderately prominent and exhibits a yellowish hue, suggestive of an older stellar population. Faint spiral arms are visible extending outwards from the central bulge, with indications of dust lanes interspersed within the arms. The arms exhibit a tightly wound morphology. Star formation activity is suggested by faint bluish regions within the spiral arms, indicative of younger, hotter stars. The overall structure seems relatively undisturbed, showing no strong signs of ongoing or recent major merging events. There is a very mild disturbance in the arms that may indicate a minor merger.
