The galaxy presents as a single, concentrated object with a generally smooth appearance. Its morphology appears elliptical, exhibiting a high degree of radial symmetry. The light distribution is centrally concentrated, with a gradual decrease in intensity outwards from the core. Color gradients are subtle, with the core exhibiting a yellowish-white hue, transitioning to a slightly redder color in the outer regions, potentially indicating an older stellar population in the outer parts of the galaxy. There is little evidence of spiral arms, a disk, or dust lanes, supporting the interpretation of an elliptical galaxy. There appears to be no significant morphological disturbance due to tidal interactions or recent mergers. The overall impression is that of a relatively quiescent system with a well-mixed stellar population.
