The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. The central region exhibits a bright, concentrated luminosity, suggesting a high stellar density, possibly indicative of a bulge. The galaxy appears largely featureless, lacking prominent spiral arms or distinct dust lanes. The outer regions gradually fade into the background sky, with a subtle color gradient suggesting a change in stellar population or composition from the core to the outskirts. There are no obvious signs of tidal disturbances or interactions with neighboring galaxies in the immediate vicinity based on the smoothness and general lack of asymmetry in the galaxy's shape. The object displays a relatively round appearance. There is no visible evidence of a strong disk component or active star formation regions.
