The galaxy presents as a smooth, centrally concentrated object. The light profile appears relatively featureless, lacking prominent spiral arms or a distinct disk. The central region exhibits a bright, yellowish hue, possibly indicative of an older stellar population. A more diffuse, bluish halo surrounds the core, suggesting the presence of a younger, bluer stellar population or ongoing star formation, albeit at a low rate. The galaxy's overall shape is close to round. There is no visible evidence of tidal disturbances or ongoing mergers.
