The galaxy appears as a relatively small, elliptical-shaped object with a smooth light distribution. It is elongated in shape, exhibiting an aspect ratio indicative of an E5 or E6 elliptical classification. Its color profile suggests a relatively older stellar population, with a bias toward redder wavelengths although some blue regions can be seen. There is no visible dust lane or spiral arm structure. The galaxy shows no signs of recent or ongoing major mergers, such as tidal tails or significantly distorted morphology, though a minor disturbance cannot be completely ruled out.
