The galaxy exhibits a smooth, elliptical morphology with a high degree of central concentration. The isophotes appear relatively regular, though a subtle asymmetry is suggested by the slight elongation along a discernible axis. Color gradients are present, with the central regions displaying a yellower, possibly redder hue, indicating an older stellar population dominated by evolved stars. The outer regions fade in intensity and appear slightly bluer, potentially indicating the presence of a younger stellar population or residual star formation activity. There is no apparent spiral arm structure or dust lanes visible, and the galaxy lacks the clumpy morphology often associated with actively star-forming systems. The overall impression is that of a quiescent, relatively evolved galaxy.
