The galaxy presents as an elongated, centrally concentrated object. It appears to be an elliptical galaxy with a smooth, largely featureless morphology. The core of the galaxy exhibits a bright, yellowish-white hue, suggesting a population of older stars. Progressing outwards from the core, the color shifts towards a faint bluish tint. This suggests the presence of younger stars, possibly indicating ongoing or recent star formation activity, albeit at a seemingly low rate. The galaxy's shape deviates significantly from a perfect sphere, with an estimated diameter of around 4 kpc. There is no apparent evidence of spiral arms, a bar structure, or any major disturbances indicative of ongoing merging events. The galaxy appears relatively undisturbed and isolated.
