The galaxy presents as an elliptical or lenticular type, exhibiting a largely smooth and concentrated morphology. It displays a dominant central bulge. Color gradients suggest a stellar population that is composed of older stars. Faint indications of a weak disk structure can be observed. There is a suggestion of a minor disturbance in the galaxy's structure, perhaps from a recent or ongoing interaction, although no substantial merger event is apparent. A slight asymmetry in the light distribution could corroborate this assessment. The galaxy appears relatively isolated, without any obvious companion galaxies or tidal features to indicate major interactions. Star formation activity appears to be low.
