The galaxy presents as a relatively compact and smooth elliptical. Its core region exhibits a strong, yellowish hue, suggesting a population dominated by older stars. Moving outwards from the core, the galaxy's color gradually shifts towards a more reddish-brown tone. This color gradient might indicate a decreasing age of stellar populations or increasing dust content in the outer regions. There is a subtle elongation to the galaxy's shape, appearing more oblate than perfectly spherical. There's no evident spiral structure, arms, or prominent dust lanes visible. No signs of ongoing major mergers or significant tidal disturbances are detected within the immediately vicinity. Overall, the galaxy appears to be a well-formed, relatively undisturbed system that is more red than blue.
