The galaxy presents a roughly elliptical morphology, appearing somewhat flattened. Its color profile suggests an older stellar population, with a dominant yellowish hue in the central region that likely corresponds to a bulge. The outer regions exhibit a slightly bluer tinge, hinting at the possibility of some ongoing, albeit subdued, star formation. The galaxy's overall structure appears relatively smooth, lacking any prominent spiral arms or distinct features that would indicate a recent major merger event. There are no signs of tidal tails or obvious distortions in its shape. There may be a very weak disk-like component in the galaxy.
