The galaxy presents as a centrally bright, elliptical structure with a smooth, relatively featureless disk. The central bulge exhibits a high surface brightness, appearing almost stellar in nature. The disk component displays a blue hue, suggesting the presence of younger stellar populations. There are faint indications of possible minor disturbances along the outer edges of the galaxy, hinting at a potential past merger event. Overall, the galaxy appears to be relatively undisturbed and exhibits characteristics of a smooth morphology.
