The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a fairly round morphology. There's a notable central bulge that is bright and concentrated, showing a yellowish hue, which might indicate an older stellar population. Moving outward from the core, there's a gradual decrease in surface brightness, transitioning into a bluer halo or disk. This could imply the presence of a younger stellar population in the outer regions, though the smoothness suggests a lack of distinct spiral arms or prominent dust lanes. There is no indication of significant tidal disturbances or ongoing mergers, although subtle asymmetry cannot be ruled out. The overall appearance suggests a galaxy that is relatively undisturbed and potentially approaching quiescence in terms of star formation.
