The galaxy presents as a somewhat smooth, elliptical-like structure. It exhibits a centrally concentrated luminosity profile. The color appears to be relatively uniform across the galaxy, with a slight reddish or yellowish hue, potentially indicating a population of older stars or a significant dust component. There are no obvious signs of spiral arms or active star-forming regions readily discernible in this image, although based on data, some star formation is indicated. The galaxy appears relatively undisturbed, lacking any major distortions or tidal features that would suggest recent or ongoing merger activity, although there may be minor disturbances.
