The galaxy appears as a single, largely featureless object with a smooth light distribution. The morphology seems to be generally elliptical, showing high degree of circularity. The color gradient indicates a dominant older stellar population, with the central region possibly containing a higher concentration of older, redder stars. There is no evidence of spiral arm structure or a prominent disk. The overall structure suggests a well-mixed system with a lack of significant ongoing star formation. There is a hint of some minor disturbances, however the galaxy mostly appears relaxed and not undergoing a major merging event. 
