The galaxy presents a generally smooth and rounded morphology, suggesting an elliptical classification. The light distribution is centrally concentrated with a bright core that diffuses outwards into a more indistinct halo. The overall color appears yellowish-orange, potentially indicating an older stellar population with minimal ongoing star formation. There is a subtle elongation, deviating slightly from a perfectly circular form, however there is no evidence of spiral arm structures or significant dust lanes within the visible light spectrum. The galaxy does not appear to be significantly interacting with any other galaxies nearby, as there are no obvious tidal tails, bridges, or distorted features. Faint hints of disturbances are present however.
