The galaxy appears as a relatively faint, moderately sized spiral structure. Its disk is not perfectly face-on but displays a slight inclination relative to our line of sight. Spiral arms are visible, though somewhat diffuse and not sharply defined. A central bulge is present, but does not dominate the overall structure. There are some slight indications of disturbances. The overall color suggests a mix of stellar populations, with some regions exhibiting bluer hues indicative of ongoing star formation, while others show more yellow/red tones, likely corresponding to older, evolved stars. The galaxy does not seem to be undergoing a major merging event.
