The galaxy presents an elliptical morphology, exhibiting a smooth, largely featureless appearance. Its overall shape suggests a deviation from perfect sphericity, showing a slightly elongated form. The central region displays a high surface brightness, indicative of a concentrated stellar population, likely composed of older stars. Moving outwards from the core, the luminosity gradually decreases, forming a diffuse halo. There is very little blue color, implying the galaxy is mostly composed of older stars with little active star formation. Overall, the galaxy appears to be a relatively undisturbed system.