The galaxy presents a primarily smooth morphology, with a subtle disk-like structure. The central bulge exhibits a bright, concentrated glow that gradually fades outwards. The disk appears somewhat inclined to our line of sight. There is an indication of a possible minor interaction or disturbance in the disk, perhaps due to a small merger event. There are hints of a faint outer halo or envelope surrounding the main body of the galaxy. The color indices suggest a relatively passive galaxy, with older stellar populations dominating the overall light.
