The galaxy presents as a spiral morphology, exhibiting loosely wound spiral arms. The arms appear somewhat flocculent and asymmetric, suggesting potential disturbances. The central bulge is moderately sized, and the disk appears relatively face-on. There is a faint suggestion of a bar structure bisecting the bulge, however this is difficult to see due to image quality. There is a noticeable interaction or merger event occurring within the galaxy, causing major disturbances to the disk structure. The overall color is indicative of a mix of stellar populations, likely indicating a recent burst of star formation activity.