The galaxy presents as a smooth, centrally concentrated object, likely an elliptical or lenticular galaxy. It exhibits a prominent bulge that is notably brighter and more luminous than the surrounding disk or halo. The light appears to gradually fade from the center outwards, suggesting a lack of distinct spiral arm structures or prominent star-forming regions. There is a subtle color gradient, with the central bulge appearing more yellow-white, possibly indicating an older stellar population. The outer regions show hints of a slightly bluer hue, but this is very faint. The overall shape is somewhat elongated rather than perfectly spherical, suggesting the galaxy is not a perfect sphere. The smooth appearance suggests that it is not currently undergoing a major merger. The galaxy shows no signs of significant disturbances such as tidal tails or shells.
