The galaxy presents as a primarily smooth, elliptical morphology with a high degree of circularity. There's a subtle color gradient, appearing slightly bluer in the central region and gradually transitioning to a redder hue in the outer halo. No distinct spiral arms or bar structures are discernible. The overall appearance suggests an older stellar population, consistent with a relatively low star formation rate. Faint tidal features are not obvious, indicating the absence of recent major mergers, although some minor disturbances cannot be ruled out. The galaxy appears relatively isolated, showing no signs of ongoing interaction with neighboring galaxies in its immediate vicinity.