The galaxy appears to be a spiral galaxy viewed at an oblique angle, somewhat inclined relative to our line of sight. The central bulge is relatively prominent and exhibits a smooth, yellowish-white hue, suggesting an older stellar population. Fainter, blue-tinged spiral arms extend outward from the bulge. There is evidence of some dust lanes within the disk. The outer regions of the disk fade gradually, suggesting the presence of an extended halo. No strong signs of active galactic nuclei or major mergers are observed. There is minor evidence of an apparent tidal tail. Star formation appears to be present, but not dominating in this galaxy.
