This galaxy exhibits a distinct spiral structure. Prominent, well-defined spiral arms are visible, tracing a path outward from the central region. The arms appear somewhat flocculent, with regions of enhanced brightness suggesting active star formation. These star-forming regions are noticeably bluer in color, indicative of the presence of young, hot stars.

The galactic bulge appears relatively small, with a moderate contribution to the overall light of the galaxy. A faint bar structure appears to be present in the central region. The disk of the galaxy is viewed at an angle. The winding of the spiral arms is relatively moderate.

Overall, this galaxy presents as a moderately sized spiral with evidence of ongoing star formation within its spiral arms. There appears to be some distortion to the galactic disk, possibly indicating an interaction with another galaxy.
