The galaxy presents as a spiral type, exhibiting a central bulge that appears relatively bright and concentrated. There is evidence of a disk component, although the spiral arms are somewhat diffuse and not sharply defined. One arm is clearly visible on the right side of the galaxy. This arm is a pale red/pink hue, and appears slightly disturbed compared to the rest of the galaxy. There are hints of blue in the outer regions of the disk, suggesting the presence of younger stellar populations or ongoing star formation, especially on the left side of the galaxy. The overall color index indicates a generally intermediate stellar population age, with a mix of both older and younger stars. Possible minor disturbance in morphology. There may be a slight asymmetry to the overall shape, perhaps due to a past interaction or merger event.
