The galaxy presents as a smooth, elliptical-like structure, exhibiting a concentrated central bulge that fades into a diffuse halo. The light profile suggests an older stellar population, as indicated by the yellowish-red hue concentrated within the galaxy's core and diminishing outwards. No distinct spiral arms or dust lanes are discernible. The shape is generally round. There is a slight elongation, but overall the galaxy lacks significant morphological disturbances or tidal features indicative of recent major mergers. Based on the color and morphology, star formation is likely suppressed.
