The galaxy appears as a centrally concentrated object with a relatively smooth, featureless morphology. Its overall shape seems elliptical, showing no obvious spiral arms or bar structures. The color profile indicates a bias towards redder wavelengths, especially within the core. This suggests an older stellar population with a lower rate of recent star formation. Faint color variations in the outer regions might be present, possibly suggesting minor dust lanes or areas of residual star formation, although the image resolution makes it difficult to confirm these features definitively. There are no apparent signs of major tidal disturbances or ongoing mergers, though the presence of a very subtle minor interaction cannot be entirely ruled out.
