The galaxy presents as a relatively smooth, elliptical object. It appears to be largely featureless, lacking prominent spiral arms or a distinct disk structure. The galaxy exhibits a centrally concentrated light distribution, with the luminosity gradually decreasing towards the outer edges. The overall shape is generally round. There is very slight asymmetry in its outer regions, possibly due to a minor gravitational interaction. Its color profile suggests a population of older stars with ongoing star formation at a very low rate.
