The galaxy presents as a spiral type, viewed at an oblique angle, not quite edge-on. A prominent central bulge is visible, appearing yellow in color, suggesting an older stellar population. Fainter, somewhat diffuse spiral arms extend outwards from the bulge. Evidence of star formation appears to be present within these arms, indicated by bluer and slightly brighter patches, though this is relatively subtle. The disk of the galaxy appears somewhat flocculent. There are also signs of a possible weak bar structure. There are no apparent major distortions indicating ongoing major merger activity. Overall the morphology suggests a moderately massive spiral galaxy with ongoing, albeit moderate, star formation.
