The galaxy presents a notable disk structure. There is evidence of spiral arms extending from a central bulge, with the arms having a somewhat flocculent appearance. The galaxy exhibits a noticeable inclination, appearing somewhat elliptical in shape. It appears to be a mostly smooth structure with a slightly brighter central region. The color distribution shows a bluer hue in the outer disk and spiral arms, potentially indicating younger stellar populations, while the central region appears relatively redder, suggesting older stars. There also appears to be a companion, possible dwarf galaxy nearby.
