The galaxy presents as a moderately luminous, elliptical morphology with a smooth appearance. The central bulge exhibits a yellowish hue, potentially indicating an older stellar population with lower rates of star formation. Fainter extensions of light are visible surrounding the central bulge, though there is a lack of prominent spiral arms. The galaxy appears generally undisturbed, with no immediately obvious signs of major mergers or tidal distortions. A slight asymmetry in the outer regions suggests a potential minor interaction or disturbance. Overall, the galaxy appears to be a relatively quiescent, evolved system.
