The galaxy presents as a roughly elliptical, disk-like structure. The central region exhibits a high surface brightness, appearing nearly uniform in color with a primarily cyan hue. The radial profile suggests a gradual decrease in luminosity from the center outwards. There is some slight asymmetry and a subtle hint of possible disturbance in the outer regions. Faint, diffuse material extends beyond the main body. There are no apparent spiral arms or prominent dust lanes visible. The color profile indicates the presence of both older stellar populations.
