This galaxy presents as a spiral with a notable disk structure. The disk exhibits a high degree of asymmetry, with a distinct spiral arm pattern. The winding of the spiral arms appears to be relatively tight in certain regions and medium-pitch in others. Distinct regions within the arms present with higher luminosity suggesting active star formation.

A central bulge is present. It appears relatively small in comparison to the disk, but it is well defined with no distinct features in this image. The light from the bulge is a yellower color compared to the disk and spiral arms, suggestive of an older stellar population.

Evidence of a bar structure is present, though it is somewhat weak. A slight perturbation or disturbance is apparent in the spiral arm structure, potentially indicating a past or ongoing minor merger event. There are no clear indications of dust lanes within the disk, but at this resolution, subtle features may be difficult to discern. The overall color of the disk suggests a relatively high rate of star formation.
