The galaxy presents as a centrally concentrated object with a relatively smooth, featureless morphology. Its overall shape appears circular, exhibiting a high degree of rotational symmetry. The light profile is centrally peaked, indicating a possible bulge component, which is expected for a galaxy of this mass. The color appears to be predominantly yellow/red, which indicates an older stellar population and potentially suppressed ongoing star formation activity. This is consistent with the observed smooth appearance, as star formation regions would likely be brighter and bluer. There may be some evidence of minor tidal disturbances in the galaxy's halo, but this is somewhat questionable due to image quality. It does not appear to be a galaxy undergoing a major merger event.
