The galaxy presents as a spiral type, seen at a slight inclination. The morphology is characterized by a prominent central bulge, with moderate size relative to the overall galactic disk. The disk component exhibits well-defined spiral arms, appearing somewhat flocculent. These arms display an average winding, and two spiral arms appear to dominate the structure. There is evidence of a bar structure across the bulge region, appearing as a central elongation. The disk exhibits both blue and red colors in spiral arms, as well as a yellow bulge. There is no apparent interaction with nearby galaxies or evidence of major merging events. There appears to be ongoing star formation activity distributed within the spiral arms. 
