The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a concentrated central bulge that gradually fades into an extended halo. The color is predominantly yellow-white, suggesting an older stellar population with fewer young, hot stars. There is a slight elongation, but overall the galaxy presents a rather regular, undisturbed morphology. There is little evidence of spiral arms or significant dust lanes. Faint hints of substructure or tidal features are not readily apparent in the image, suggesting the galaxy is likely not undergoing any major merger events. The galaxy exhibits a compact structure, with the bulk of its light concentrated in a relatively small area.
