The observed galaxy presents a slightly elliptical morphology, suggestive of either an elliptical galaxy or a spiral galaxy viewed at a significant inclination. The central region exhibits a high degree of luminosity and a yellow/white hue, possibly indicating an older stellar population or a strong concentration of dust. Diffuse, fainter extensions are visible surrounding the central region, exhibiting a bluer color. The blue extensions may indicate ongoing or recent star formation within the galaxy. There is a very faint, almost indistinguishable disk in the galaxy with some irregularities. There is no distinct dust lane or other clear features that would allow for a definitive classification based on this image alone. The overall structure appears relatively undisturbed, without any obvious signs of major mergers or tidal interactions.
