The galaxy appears as a centrally concentrated object, generally smooth in texture. A slight elongation is noticeable, deviating from a perfectly circular shape. The core exhibits a bright, yellowish-white hue, suggesting an older stellar population dominating the nuclear region. Fainter, more diffuse extensions are visible surrounding the central bulge, showing a reddish tint. These features could indicate regions of on-going, albeit subdued, star formation. There is a slight indication of asymmetry, suggesting possible gravitational interaction or a minor disturbance. Overall, the galaxy presents characteristics consistent with an elliptical or lenticular galaxy at a substantial distance.
