The galaxy presents as a relatively smooth, elliptical-like structure, though subtle irregular features are discernible. A bright central bulge is evident, exhibiting a yellowish hue, suggesting a population of older, redder stars. The outer regions of the galaxy display a bluer tint, which may indicate ongoing or recent star formation. The overall form appears mostly round. There seems to be some minor disturbance to the disk, possibly implying a past or ongoing interaction with another galaxy.
