The galaxy presents as a centrally concentrated, relatively smooth object. Its shape is approximately round, exhibiting minimal deviation from circular symmetry. There is some evidence of minor disturbances or subtle features within the galaxy's structure. It exhibits a moderate level of star formation activity, inferring the presence of both younger, bluer stellar populations and older, redder stars. The galaxy appears to be a fairly massive system. There is no obvious sign of interaction with other galaxies or of major ongoing mergers.
