The galaxy appears to be a spiral galaxy, albeit somewhat face-on. It exhibits a central bulge region with a reddish hue, suggesting an older stellar population. Fainter, bluer spiral arms extend outward from the bulge. These arms are not sharply defined, hinting at a lower density of star formation. The galaxy appears somewhat elongated. There are no readily apparent signs of a major ongoing merger, though there might be minor disturbances to the overall structure. The galaxy appears relatively smooth. Overall the galaxy presents a moderate mass. Its star formation rate appears to be relatively low.
