The galaxy appears as a fairly smooth, centrally concentrated object. Its morphology leans toward elliptical, with a generally round shape, although with some departure from perfect circularity. There is no obvious spiral structure, and it lacks prominent features such as a distinct disk or bar. 

The galaxy's color profile suggests a dominant population of older stars. It has a central bright yellowish-white core which may indicate a concentration of older stars. The overall impression is of a relatively quiescent galaxy with little ongoing star formation. However, there are hints of blue in the outskirts, possibly indicating a minor population of younger stars. There are no obvious signs of a major merger event, though a slight asymmetry could suggest past interactions or a minor disturbance.
