The galaxy presents as a relatively smooth, elliptical structure, with a high degree of central concentration. The light profile suggests a prominent bulge component, with a gradual decline in surface brightness moving outward. There's no clear evidence of spiral arms or a distinct disk. The overall color appears to be yellowish-white, indicating an older stellar population and a lack of significant ongoing star formation. The shape is mostly rounded with a slight elliptical distortion. There are no signs of major mergers or significant tidal disturbances in the immediate vicinity. Some minor asymmetry may be present, although the resolution limits a more detailed assessment of any internal structures.
