The galaxy appears as a centrally concentrated, smooth object, with a slight elongation but tending towards a circular appearance. Its color profile suggests a population dominated by older stars. The lack of discernible spiral arms or dust lanes supports its classification as an elliptical or lenticular galaxy. There's a very slight color gradient, with the core appearing marginally bluer than the outer regions of the halo, potentially indicating some degree of ongoing, albeit low-level, star formation. There is no major disturbances and it appears to be undisturbed.
