The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears to be elliptical, with a noticeable lack of spiral arms or a distinct disk structure. The color profile suggests an older stellar population, dominated by redder wavelengths, indicating a lower rate of current star formation. A slight asymmetry may suggest a minor tidal disturbance. The size is moderate, and a lack of intense features or distortions suggests that this is a relatively evolved galaxy.
