The galaxy presents as a spiral type, with a moderately sized bulge that constitutes a significant portion of its overall structure. Two prominent spiral arms emanate from the central bulge, exhibiting a tightly wound morphology. The arms appear relatively symmetric and trace a fairly regular spiral pattern. The galaxy is not oriented perfectly face-on; there is a slight tilt, allowing for the discernment of a flattened disk structure. No signs of ongoing major mergers are immediately apparent, though there is a hint of a minor disturbance in the galaxy's disk.  The light distribution within the galaxy shows a concentration towards the center, which diminishes steadily towards the outer regions. The colors appear bluer in the disk, particularly in the spiral arms, suggesting the presence of young, hot stars and ongoing star formation activity. A faint bar-like structure is present in the center region.