The galaxy presents as a relatively smooth, elliptical structure with a high degree of central concentration. The core region exhibits a bright, yellowish-white hue, indicative of a population of older stars. This bright central bulge fades gradually into a more diffuse halo. The overall shape is more 'in-between' round and elliptical. There is no obvious spiral structure, dust lanes, or other features typically associated with actively star-forming galaxies. The galaxy does not show signs of a major disturbance, such as tidal tails or asymmetries, but there is the possibility of minor disturbances. The color gradients suggest some variation in stellar populations, potentially with a younger stellar population in the outer regions contributing slightly bluer light. The size appears moderately large and suggests an average size for an elliptical galaxy at its distance. The faintness of the outer regions indicates a low star formation rate.
