The galaxy presents as a somewhat face-on spiral galaxy with a moderate central bulge. Evidence of spiral arm structure is visible, albeit somewhat diffuse, suggesting flocculent arms. The core region is bright and concentrated, exhibiting a yellow-orange hue, consistent with an older stellar population. The spiral arms appear bluer, indicative of ongoing star formation. The galaxy shows signs of a weak bar structure. There is no strong indication of any major mergers or strong disturbances to the galaxy's morphology.
