This galaxy appears to be a spiral galaxy viewed at a significant inclination, possibly nearing edge-on. It exhibits a moderately bright central bulge, from which fainter, bluish spiral arms extend. The arms display some patchiness, suggesting areas of active star formation within the disk. There appears to be some level of distortion. No clear, major merger is apparent, though there may be some minor interaction or disturbances affecting its structure. Overall the galaxy appears to be a relatively normal, star-forming spiral galaxy.
