This galaxy exhibits a smooth, centrally concentrated morphology, suggesting an elliptical or lenticular classification. The galaxy presents a slightly elongated shape, not perfectly spherical, but tending towards roundness. The core appears quite luminous and is surrounded by a more diffuse halo or envelope of stars. There is a subtle color gradient, with the central region showing a yellower or redder hue compared to the outer regions. There is little evidence of spiral arms, significant dust lanes, or major disturbances indicative of recent or ongoing mergers. The general structure implies a relatively evolved stellar population and a quiescent star formation rate. Subtle irregularities in the outer regions are present, possibly suggesting minor interactions or past merger events.
