The galaxy presents as a moderately sized, elliptical-type object. The light profile appears relatively smooth and centrally concentrated, with a gradual decrease in luminosity moving outwards from the core. The central region exhibits a yellowish-white hue, suggesting a population of older stars. The galaxy displays a relatively round morphology, with no apparent strong disk features or spiral arms. There is no readily obvious evidence of ongoing major mergers or tidal disturbances in its overall structure. The object appears largely undisturbed. The light is most concentrated in the green and red wavelengths. There is a degree of star formation. The mass is approximately 10^10 solar masses. 
