This galaxy appears to be a relatively smooth elliptical galaxy, exhibiting a concentrated central bulge that fades into a more diffuse halo. There's a slight elongation, but overall the shape is more or less spheroidal. The color gradient suggests older stellar populations, with a yellowish-orange hue in the center that might indicate a lack of significant ongoing star formation. We see a very smooth, continuous falloff in brightness from the core of the galaxy to its faint outer edges. There isn't evidence of significant dust lanes or spiral arm structures. The overall appearance suggests that any recent or major merger events are unlikely, with perhaps only minor disturbances to the galaxy's morphology.
