The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a bright, yellowish-white luminosity that decreases in intensity towards the outer regions. A subtle bluish halo surrounds the central region, suggesting the presence of a younger stellar population. The galaxy appears relatively undisturbed, without prominent tidal features or asymmetries indicative of recent major mergers, though there may be minor irregularities in the outer isophotes. Overall, it seems to be a galaxy with characteristics of a spheroidal system with some evidence of star formation.
