The galaxy exhibits an elliptical morphology with a smooth light distribution, indicating a dominant spheroidal component. It shows a slight elongation, suggesting it is not perfectly spherical. The galaxy presents a concentrated core with a gradual decrease in luminosity towards its outer regions. Faint tidal features or distortions are not readily apparent, implying a relatively undisturbed structure or past interactions. The color profile suggests a population of older stars, as the core is yellowish-white. No prominent dust lanes or spiral arm structures are detected, reinforcing its classification as an elliptical galaxy.
