The galaxy presents a primarily smooth, elliptical morphology. It exhibits a concentrated central bulge that appears nearly spherical in projection. The color profile is generally consistent, with a slight redder hue concentrated in the core region, fading to a bluer tone in the outer edges. This suggests potential differential stellar populations, where older, redder stars are concentrated in the core, and younger, bluer stars reside in the outer regions. There is no clear evidence of spiral arm structure or a prominent disk. There are no indications of major ongoing mergers or tidal disturbances, with little morphological asymmetry. Overall, the galaxy appears to be an evolved system, possibly undergoing reduced star formation.
