The galaxy presents a largely smooth morphology. It exhibits a centrally concentrated, bright core that appears nearly spherical. The light profile diffuses outwards from the core, decreasing in intensity. No distinct spiral arms or bar structures are visible, suggesting a classification toward the elliptical end of the Hubble sequence or possibly a lenticular galaxy. The color appears to be a yellowish-white, indicating a population of older stars. There are no significant signs of dust lanes or active star formation regions within the visible light. There's a slight elongation to the shape, neither perfectly round nor highly elongated. Subtle disturbances or faint tidal features might be present in the outer regions, which could suggest a past minor merger event, but the overall structure is primarily undisturbed.
