The galaxy appears to be a relatively smooth, elliptical-like structure, with a bright, concentrated central bulge. The light profile suggests a gradual decrease in luminosity from the center outwards.  There is a slight hint of a disk-like component surrounding the central bulge, however it's very dim. The overall color is yellowish-orange, indicating an older stellar population and a lack of significant ongoing star formation. There may be some very slight disturbances in the outer regions of the galaxy, but it doesn't appear to be undergoing any major mergers or interactions.  The galaxy exhibits a generally rounded morphology.
