The galaxy appears to be an elliptical galaxy, or potentially a lenticular galaxy seen face-on. It exhibits a smooth, diffuse light distribution. The central region is brighter and has a yellow hue, suggesting an older stellar population. The outskirts of the galaxy appear less luminous and have a slightly bluer tint, potentially indicating the presence of some younger stars or a lower metallicity stellar population. The overall shape appears mostly round. There is no clear evidence of spiral arms, a central bar, or any significant tidal disturbances indicative of a recent merger event. The galaxy seems to be relatively isolated and undisturbed.
