The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. The light profile suggests a spheroidal distribution of stars. The core region exhibits a yellowish hue, implying an older stellar population. There is a lack of discernible spiral arms or prominent dust lanes, furthering the classification as an elliptical galaxy. The overall appearance is indicative of a relatively evolved system, with low levels of ongoing star formation. The outer regions appear slightly bluer than the core, which may suggest a population of younger stars residing on the outskirts. There is no visual evidence of tidal features or ongoing merger activity, suggesting this is a relaxed, isolated system.
