The galaxy appears to be a spiral galaxy, presented at an angle that is slightly inclined from a face-on orientation. It exhibits a prominent disk structure. Spiral arms are visible, though they are not sharply defined. The bulge component is moderately sized, showing a concentrated central region. The presence of a bar feature is also indicated in the structure.

There is evidence of ongoing star formation, as suggested by the patchy distribution of light within the spiral arms and the overall color profile. The galaxy does not appear to be undergoing a major merger, though some minor disturbances cannot be ruled out. Overall, the galaxy presents a typical spiral morphology with signs of active stellar processes.
