The galaxy appears to be a spiral type with a relatively bright, centrally concentrated bulge. The disk is observed nearly edge-on. There are faint, diffuse extensions emanating from the central region along the major axis, possibly indicative of a tidal disturbance or ongoing merger event. The central region exhibits a blue hue, which might suggest recent star formation activity. The outer regions of the disk show a greenish tint that indicates the presence of older stellar populations. Patches of red and blue light are scattered throughout the galaxy, which is indicative of star forming regions. The overall morphology is complex, suggesting a possible interaction with another galaxy or past mergers. 
