The galaxy appears as a moderately inclined, somewhat diffuse spiral. It exhibits a faint central bulge region that transitions smoothly into a disk. There is evidence of spiral arm structure, although it is not sharply defined; the arms are rather flocculent and fragmented, presenting as subtle variations in surface brightness across the disk. A bluer hue is noticeable along these arm segments, suggestive of ongoing star formation, particularly in the disk region. There are some disturbances that can be noticed in the spiral arms, which are lumpy in appearance, hinting that there may have been an event that distorted the galaxy's structure. Overall, the galaxy presents a relatively low surface brightness and moderate redshift, implying that it is at a significant distance.
