The galaxy presents as a moderately bright object of an elliptical morphology. It displays a high degree of symmetry, with no apparent spiral arms or bar structure. There is no clearly visible nucleus. The galaxy exhibits a smooth light distribution, with minimal evidence of internal substructure or dust lanes. The color appears relatively uniform, with the light being slightly more blue than red. The presence of a smooth profile, elliptical shape, and the uniform color suggest a population dominated by older stars with ongoing or recent star forming activity. There appears to be a slight asymmetric feature, or merging component. No major distortions or tidal tails are readily observed.
