The galaxy appears to be a moderately bright spiral galaxy, seen at an inclined angle. The central bulge presents a reddish hue, possibly indicating an older stellar population. A faint disc structure is apparent, showing some blue-green coloring, which could be indicative of ongoing star formation. The overall shape is somewhat elongated. There is some evidence of possible minor disturbances in the spiral arms, but there is no clear indication of a major merger event or a strong interaction with another galaxy. The galaxy appears relatively isolated.
