The galaxy presents as a spiral galaxy with an inclination that allows for a clear view of its structure. Two prominent spiral arms are visible, exhibiting a medium to loose winding pattern. The central bulge appears to be of moderate size relative to the disk. There is no indication of a strong bar structure. The galaxy appears to be undergoing a merging event or interacting with another galaxy, evidenced by some degree of morphological disturbance or tidal features. Based on the color indices, the galaxy is actively forming stars.