The galaxy presents as a centrally concentrated object with a smooth, relatively featureless morphology. The light distribution suggests an elliptical shape, appearing elongated with a moderate ellipticity. A color gradient is observed, with the core exhibiting a yellowish-orange hue, which may indicate an older stellar population. The outer regions appear fainter and slightly bluer, suggesting a younger stellar population and/or some ongoing star formation, albeit at a modest rate. There's no discernible spiral arm structure or bar feature visible in this image. The overall appearance indicates a galaxy that is not undergoing any major merging events or strong tidal interactions.
