The observed galaxy appears to be of elliptical morphology, exhibiting a generally smooth, featureless structure. The central bulge is bright and relatively well-defined, decreasing in intensity towards the outer regions. The shape is not perfectly spherical, showing a moderate elongation, appearing slightly oblate. There is some indication of possible tidal interactions or an ongoing merger event. A secondary, smaller, and less luminous concentration of light appears attached to the main galactic body. The galaxy's color profile shows it is rich in older stars, a characteristic yellow-orange hue dominates. The overall impression suggests an evolved system possibly nearing the final stages of a galactic merger.
