The galaxy presents a generally smooth, elliptical morphology. The light distribution appears concentrated towards the center, suggesting a prominent bulge. It exhibits a yellow-orange hue, potentially indicating an older stellar population with fewer young, massive stars and dust. There are no spiral arms or significant dust lanes visible. The galaxy's shape is approximately round. The overall appearance is consistent with an early-type galaxy that is not currently undergoing major merging activity. The lack of distinct features suggests that star formation is likely occurring at a moderate rate. There may be some minor tidal disturbances but the features aren't quite clear. 
