The galaxy presents a prominent disk-like morphology, oriented at an angle relative to our line of sight, approaching an edge-on configuration. The galaxy exhibits a noticeable bulge, though not overwhelmingly dominant. 

The light distribution shows variations across the galactic structure. The central region is noticeably brighter, while towards the periphery, the intensity gradually decreases. There appears to be a distinct dust lane obscuring a portion of the galaxy, possibly within the galactic plane. The galaxy's color suggests active star formation, which is corroborated by blue-ish tones in the arms. The galaxy also presents some distorted features that may indicate a possible past merger. 
