The galaxy exhibits a morphology consistent with a spiral type. A prominent central bulge is observed, with a moderate amount of light concentrated there. Faint, extended spiral arms emerge from the central region, displaying a somewhat flocculent structure. The spiral arms are observed with a winding tightness that appears to be of medium grade, not tightly wound nor loosely arranged. These structures exhibit areas of star formation, evidenced by some degree of bluer light. Dust lanes can be observed along certain parts of the arms, but are not strong. There are two dominant spiral arms that can be seen. The galaxy's overall shape is that of a spiral galaxy with no major disturbances and no major mergers. The color distribution suggests ongoing star formation, although it is moderate. The object presents a moderate degree of inclination relative to our line of sight.
