The object appears to be a spiral galaxy, observed at an angle somewhat close to edge-on. Evident dust lanes are visible along the galactic plane. The central bulge is prominent and exhibits a yellowish hue, potentially indicative of an older stellar population. Spiral arms are observable, though their morphology is somewhat difficult to discern given the viewing angle. Based on the prominence of the disk relative to the bulge, this galaxy is likely a late-type spiral. A bar structure is not immediately apparent, but it may be present. The spiral arms appear to have a tight to medium winding, and are likely moderately numerous. There is no obvious evidence of a major merger or significant tidal disturbances. The outer regions of the disk show a bluer color, suggesting more recent star formation is taking place there.
