The galaxy presents a largely smooth, elliptical morphology, with a concentration of light towards its center. The core exhibits a yellowish-orange hue, which may indicate a population of older stars. A subtle gradient transitions outward from the core to a fainter, greenish-blue halo. This outer region could suggest the presence of a younger stellar population or ongoing star formation, although it is not particularly pronounced. There are no apparent spiral arm structures or significant dust lanes visible. The galaxy appears relatively undisturbed, showing no strong signs of tidal interactions or recent major mergers, although there is potentially minor evidence of gravitational disturbance in the outer halo. The overall shape is nearly round, with only a slight deviation toward a cigar shape. Based on the observed color gradients and smooth morphology, this galaxy could represent an elliptical galaxy undergoing some degree of recent or ongoing star formation.
