The galaxy presents as a relatively smooth, disk-dominated spiral with a noticeable central bulge. The color profile suggests an older stellar population, particularly within the bulge, which appears more yellow. The spiral arms are not sharply defined, appearing somewhat flocculent and blended into the overall galactic structure. There is little evidence of active star formation regions, as indicated by a lack of prominent blue coloration. The galaxy displays a moderate inclination, allowing for some visualization of its disk shape. There may be some minor disturbances in the outer disk region, as suggested by slight irregularities in its shape. It appears to be a relatively massive galaxy. Overall, the morphology is suggestive of a galaxy undergoing a relatively quiescent period of star formation.
