The galaxy presents as a relatively smooth, elliptical-like structure. The light distribution suggests a centrally concentrated bulge with a gradual decline in surface brightness towards the outer regions. There is a faint suggestion of a disk, or spiral arm structures, but they appear faint. The galaxy exhibits a yellow-orange hue, which suggests an older stellar population with less active star formation. There appears to be no central active galactic nucleus, based on the smooth light profile and lack of significant blue color in the center. Some minor tidal disturbances cannot be ruled out, but there is no major disturbance or sign of merging activity apparent. The object appears to be an isolated galaxy.
