The galaxy exhibits a spiral morphology, with discernible arm structures emanating from a central bulge. The spiral arms appear somewhat tightly wound. There is some evidence of a bar-like structure in the central region. The bulge is moderately sized relative to the disk. Patches of star formation are visible within the spiral arms, indicated by bluer regions. There may be some minor disturbances present in the galaxy's morphology, potentially indicating past or ongoing interactions. The galaxy's overall color is yellowish, suggesting a significant population of older stars. The mass is estimated to be fairly high, suggesting a relatively massive galaxy. There is evidence of ongoing star formation.
