The galaxy presents as a somewhat elongated, moderately luminous structure with a smooth, elliptical morphology. There is a central concentration of light that fades gradually outward, indicating a likely bulge component. The overall color appears yellowish-orange, suggesting an older stellar population with a reduced rate of recent star formation. No distinct spiral arms or significant dust lanes are discernible within the observed features, reinforcing the classification as an elliptical or lenticular galaxy. There are no clear signs of any recent or ongoing major merging activity or tidal disturbances. It appears to be a relatively undisturbed system.
