The galaxy presents as a centrally concentrated, elliptical structure with a smooth, diffuse light profile. The core region exhibits a yellowish-white hue, suggesting a population of older stars. A gradual color gradient is observed moving outward from the core, transitioning to a slightly redder shade in the outer regions. The overall morphology suggests a relatively undisturbed system, with no obvious signs of ongoing major mergers or tidal interactions. There might be some minor disturbances within the structure, but this is difficult to say for sure given the image's resolution. The galaxy appears generally round in shape, with a slight elongation noticeable along one axis. There is no apparent dust lane or spiral arm structure visible. Overall, the galaxy appears to be a fairly massive, evolved system, with a relatively low rate of star formation.
