The galaxy presents a generally smooth, elliptical morphology. It displays a concentrated central bulge with a fairly diffuse outer halo. Color gradients are apparent, with the central region exhibiting a more yellow hue, suggesting an older stellar population. The outer regions appear slightly bluer, potentially indicating younger stars or some ongoing star formation, though at a relatively low rate. There is no prominent disk structure visible. The overall impression is that of a mature galaxy, likely with a substantial stellar mass. There are no obvious signs of recent major merger activity or significant tidal disturbances.
