The galaxy presents as a relatively smooth, centrally concentrated object. Its overall morphology is elliptical, appearing somewhat flattened rather than perfectly spherical. There is a noticeable color gradient, transitioning from a reddish core to a greenish-yellow outer region. This suggests potential differences in stellar populations and/or dust content between the central bulge and the outer parts of the galaxy. There is no obvious evidence of strong spiral arm structure or a prominent disk. The overall appearance indicates that it could be in a relatively quiescent state, potentially an evolved galaxy with a reduced rate of star formation. There are no obvious signs of major mergers or strong tidal disturbances. The relative smoothness implies that the galaxy's light is dominated by an older stellar population.
