The galaxy appears to be an elliptical galaxy, classified as smooth and not displaying prominent spiral arms or a significant disk-like structure. The light is concentrated in the center, with luminosity decreasing radially outwards.

The central region is a bright, yellowish-white color, indicative of an older stellar population. The outer regions show a somewhat redder hue, which is often associated with older, cooler stars and lower levels of star formation. 

There are no obvious signs of dust lanes or active star formation regions. No significant tidal features or distortions are observed, suggesting that it has not undergone a recent major merger. The overall structure is relatively symmetrical, with a slight elongation. 
