The galaxy appears to be an elliptical type, exhibiting a generally smooth morphology. The light profile displays a high degree of central concentration, with a bright, yellowish core. The shape is roughly elliptical, with the semi-major axis oriented vertically. There is little evidence of spiral arms or prominent dust lanes. The outer regions of the galaxy exhibit a gradual decrease in surface brightness, suggesting a diffuse stellar halo. No signs of ongoing major mergers or tidal disturbances are evident, and the overall impression is of a relatively undisturbed system. The color indices suggest a population of older stars dominates the light output.
