The galaxy presents as an elliptical morphology with a smooth light distribution. A distinct central bulge is evident, exhibiting a yellowish hue, potentially indicating a population of older stars. Fainter, bluer outskirts suggest the presence of some younger stars, though the overall star formation appears to be low. There is some visual evidence of gravitational interaction or minor disturbances, as the shape is slightly asymmetric. There are no distinct tidal tails or other obvious signs of a major merger event.
