The galaxy presents as a centrally concentrated object, appearing largely smooth and spheroidal in shape. The core exhibits a bright, yellowish hue, suggesting a population of older stars. There is a slight elongation observed, moving away from a perfectly round shape. Subtle color variations are present, with hints of bluer light towards the periphery on one side of the galaxy and redder colors on the other. The overall structure appears relatively undisturbed, showing no major signs of ongoing mergers or significant tidal distortions, though there may be some minor interaction or disturbance present, given the non-uniform color distribution. Overall, the galaxy appears as an elliptical galaxy, likely a significant mass, with a relatively low star formation rate.
