The galaxy presents as a moderately luminous, early-type system exhibiting a high degree of central concentration. The light profile appears smooth and elliptical with a suggestion of slight elongation. Color gradients suggest a population dominated by older stars, exhibiting a redder color toward the center and subtly bluer hues in the outer regions, possibly indicating residual or recent low-level star formation. There is no obvious indication of spiral structure or a prominent disk component, nor are there indications of any major ongoing mergers or tidal disturbances. The galaxy's morphology is consistent with a lenticular or elliptical classification.
