The galaxy presents as a moderately luminous system with an overall elliptical morphology. The central region exhibits a bright, concentrated core, suggesting a significant stellar density and possibly the presence of a supermassive black hole. A smooth, extended halo surrounds the core, indicating an older stellar population. There is some asymmetry in the outer regions of the halo, possibly due to minor tidal interactions or past merger events. The galaxy does not show any strong evidence of spiral arm structure or active star formation within the visible spectrum. The overall color appears relatively red, consistent with a population of older, cooler stars, though there are some hints of slightly bluer areas mixed in. The system is not obviously disturbed, though deeper observations would be needed to assess this more fully.
