The galaxy presents an elliptical morphology, with a smooth, featureless structure dominating its overall appearance. The core exhibits a high degree of central concentration, indicated by a bright, concentrated luminosity gradient. The light profile gradually decreases towards the outer regions, where a hint of a faint disk or extended halo may exist.

Color analysis reveals a predominantly yellowish-red hue concentrated in the core region. This color suggests an older stellar population is concentrated in the core. The outer regions appear slightly bluer.

There are no apparent signs of spiral arms or significant dust lanes. Evidence of tidal disturbances or ongoing major mergers seems absent, though a minor perturbation cannot be entirely ruled out. The galaxy's apparent axial ratio indicates a moderately flattened ellipsoidal shape, not far from being spheroidal.
