The galaxy presents as a smooth, elliptical structure, with a high degree of central concentration. The luminosity profile appears relatively uniform, lacking any distinct spiral arm features or prominent dust lanes. Its shape is elongated, appearing more cigar-shaped than circular. Color gradients are subtle; a slight blueish hue is observed within the central region. Overall, the morphology suggests an evolved stellar population with a modest rate of on-going star formation. There appears to be no signs of major mergers or significant tidal disturbances in the immediate vicinity, indicating a relatively undisturbed evolutionary history.