The galaxy presents as a moderately sized spiral system, exhibiting a disk structure with a non-negligible central bulge. The spiral arms appear somewhat flocculent and ill-defined, lacking sharp boundaries. Their color suggests ongoing star formation. The overall color is slightly blue-ish with signs of dust lanes. There is evidence of mild interaction or tidal features around the outer regions of the galactic disk, suggesting possible gravitational interactions. There may be a merger in progress, and the galaxy shows minor or major disturbances. The galaxy is unlikely a smooth elliptical system.
