The galaxy presents as a centrally concentrated, luminous object with a diffuse, extended halo. The primary color appears to be a yellowish-orange, indicating a population of older stars and a lack of significant ongoing star formation. The morphology is generally smooth, with a slight elongation along one axis suggesting a possible elliptical or lenticular classification. There are no visually discernible spiral arm structures or dust lanes. No signs of tidal tails, merging features or strong gravitational distortions are observed.
