The galaxy presents as a spiral type, displaying a clearly defined disk structure. A prominent central bulge dominates the galaxy's core, exhibiting a relatively smooth texture and a yellowish-white color indicative of an older stellar population.

Spiral arms are visible, exhibiting a somewhat flocculent structure. The arms appear tightly wound, originating near the central bulge and extending outwards. The arms show hints of blue coloration, suggesting regions of active star formation, although the overall color of the disk leans towards a yellow-white hue, implying a moderate level of ongoing star formation. Dust lanes can be observed, particularly along the inner edges of the spiral arms, contributing to the irregular appearance. There is the appearance of a bar in the center of the galaxy.

The galaxy does not display any obvious signs of a major ongoing merger, although some minor asymmetries in the spiral arm structure might suggest past interactions or minor disturbances. There is the appearance of a smaller disturbance on the top right of the galaxy's disk.