The galaxy presents a predominantly elliptical morphology, exhibiting a smooth, diffuse light distribution. The core is bright and concentrated, with luminosity gradually decreasing towards the outer regions. The galaxy appears elongated with a slight deviation from a perfectly circular shape. There is no obvious dust lane or spiral arm structure visible. The color profile suggests an older stellar population, as indicated by the yellowish-white hue, particularly in the central bulge. Outer regions exhibit a bluer tint. There are no discernible signs of active galactic nuclei activity or significant star formation regions from visual inspection alone. Overall, the galaxy appears relatively undisturbed, showing no major signs of recent mergers or tidal interactions.
