The galaxy presents as a relatively smooth, elongated structure. The color is dominated by a yellowish-orange hue, which suggests an older stellar population, potentially with fewer ongoing star formation regions. The galaxy's morphology appears mostly undisturbed, with no obvious signs of major mergers or significant tidal disruptions. There is a slight indication of asymmetry but it's very subtle. The central region appears slightly brighter than the outer regions, indicating a possible concentration of stars and/or a modest active galactic nucleus. Overall, the galaxy appears to be a relatively evolved system, likely an elliptical or lenticular galaxy at a considerable distance.
