The galaxy presents as a somewhat elliptical, smoothly distributed light source. The light profile appears centrally concentrated, with a gradual decrease in intensity towards the outer regions. The core region appears a yellow-white hue, which could suggest a population of older stars, with the outer regions showing a slight blue tint. The overall shape is not perfectly spherical, leaning towards a more oblate spheroid appearance. No distinct spiral arms or well-defined features are readily apparent, indicating a generally homogenous structure. There are no apparent major disturbances.
