The galaxy appears as a centrally concentrated system with a smooth, elliptical morphology. It exhibits a pronounced central bulge that is slightly brighter and more concentrated than the surrounding disk. The disk component appears relatively featureless with no clearly defined spiral arm structure. The color profile suggests a moderate population of older stars, with a general lack of bright blue regions indicative of recent star formation. There is a slight asymmetry in the outer regions. The overall structure suggests a galaxy that is in a relatively quiescent state, with a possible merger event in its past.
