The observed galaxy presents as a spiral galaxy, viewed at a significant inclination.  The central bulge appears moderately sized and bright, with a generally smooth appearance. Faint, diffuse spiral arms are observed extending outwards from the central bulge, exhibiting some patchy regions of enhanced luminosity, suggestive of active star formation regions. The disk appears fairly thin. There is no strong bar structure visible, nor any obvious signs of a major merger event.  The overall color of the galaxy is slightly blue, which is consistent with ongoing or recent star formation. There is no clear dust lane visible. The outer regions of the galactic disk appear somewhat disturbed, possibly indicating a minor interaction or ongoing accretion.
