This galaxy presents a generally smooth and elliptical morphology. The central region exhibits a high degree of luminosity, appearing almost uniformly bright. Moving outwards from the center, the light gradually diminishes. The overall shape can be described as somewhere between round and elliptical, with a slight elongation. A minor dust lane or tidal feature appears to be extending from the galaxy. There are no apparent spiral arms or significant substructure discernible. Given the smooth appearance and lack of intense star formation, this galaxy is likely an elliptical galaxy with an estimated stellar mass in the range of 10^9 solar masses. The colors suggest a more evolved stellar population. There are no signs of major merger activity or significant disturbance to the overall structure, though some tidal disturbance may be evident.
