The galaxy presents as a spiral type, exhibiting a prominent central bulge that appears bright and somewhat amorphous. Faint spiral arms extend from the central bulge. These arms display a relatively open winding pattern and are defined by subtle variations in color and texture rather than sharply delineated boundaries. There is morphological evidence of a bar structure that traverses its central region, with indications of disturbances throughout the entire galaxy. The disk component is the most prominent and highly defined aspect of the galaxy. The galaxy exhibits a disk-like structure, with a slight inclination relative to our line of sight.
