The galaxy presents as a single, concentrated luminous object. The overall morphology appears relatively smooth and elliptical, with no discernible spiral arms or bar structures visible at this resolution. The light profile is centrally concentrated, with a gradual decrease in luminosity towards the outer regions. The core exhibits a yellowish hue, possibly indicating an older stellar population. The outer regions show a slight reddening effect, which may be caused by dust attenuation. The object does not show any obvious signs of tidal disturbances or interactions with nearby galaxies. The galaxy displays a high degree of central symmetry, with an approximate circular shape. There are no readily apparent star-forming regions visible within the galaxy. Overall, the galaxy appears to be an early-type galaxy, likely an elliptical, in a relatively quiescent state.
