The galaxy presents as a relatively smooth, elliptical-like structure. It appears largely spheroidal, with a concentrated central bulge that emits strongly in the yellow-red wavelengths, suggesting an older stellar population. The overall shape is notably round. There's a gradual decrease in light intensity moving outward from the core, with a faint, diffuse halo. The lack of distinct spiral arms or prominent dust lanes suggests a well-mixed interstellar medium. There's no evidence of tidal tails or significant distortions, indicating minimal recent interaction with other galaxies. The color profile indicates a lack of active star formation in the main body of the galaxy. Overall, the galaxy presents as a passively evolving system.
