The galaxy presents as a roughly elliptical form, with a noticeable central bulge that appears bright. The morphology displays characteristics intermediate between a spiral and an elliptical galaxy, potentially indicating a lenticular (S0) classification. There appears to be a disk component, viewable almost edge-on. The overall color index suggests a mixture of stellar populations. The central region appears bluer, possibly indicating ongoing star formation activity. Evident disturbances in the disk morphology suggest minor gravitational interactions, potentially either a merger or a fly-by. Luminous emission extends from the main body of the galaxy. 
