The galaxy presents as an elliptical system with a relatively smooth light profile. The central region exhibits a high surface brightness, indicating a dense concentration of stars. Moving outwards, the light intensity gradually decreases, forming a diffuse halo. There is no discernible spiral arm structure or dust lane obscuration visible within this image, further supporting an elliptical classification. The galaxy appears to be somewhat spheroidal in shape, with a slight elongation along one axis. The overall color is relatively uniform, suggesting a population of older stars dominating the light output. There are no obvious signs of ongoing major mergers or significant tidal disturbances.
