The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The color profile suggests a moderately evolved stellar population, exhibiting a yellow-red hue in the core possibly indicative of older stars. A gradual shift towards bluer tones is observed in the outer regions. This might point towards ongoing, though subdued, star formation activity there. The overall morphology does not reveal any apparent major disturbances or tidal features, which indicates that it might have had a somewhat quiescent evolutionary history, without recent major mergers. The roundness of the morphology suggests it could be closer to an E2 galaxy.
