The galaxy presents as a relatively smooth, elliptical object with a concentrated central bulge. The core exhibits a yellowish-orange hue, indicative of an older stellar population. Surrounding the core is a fainter, more diffuse halo, showing a slight greenish tint, possibly indicating the presence of some younger, hotter stars or ionized gas, though star formation is likely subdued overall. There is no discernible spiral structure or significant dust lanes visible within the galaxy. The galaxy appears mostly undisturbed, showing no signs of a recent major merger, though there is a possibility of a very minor disturbance based on subtle asymmetries in the outer halo. The overall morphology is consistent with an early-type galaxy, likely a lenticular or elliptical galaxy at a considerable distance.
