The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a centrally concentrated luminosity profile with a noticeable decrease in brightness towards its outer edges. The galaxy has a distinct yellow-orange hue in its central regions, suggesting a population of older, cooler stars. There is a slight indication of bluer color in the outer edges of this galaxy, suggesting the presence of some star formation. There are no obvious signs of spiral arms or a well-defined disk structure, nor any evidence of major mergers or tidal disturbances. Its shape appears to be closer to in between round and cigar-shaped with a more undefined distribution of stars at its edges.
