The galaxy appears to be an elliptical galaxy, exhibiting a smooth, featureless morphology with a generally elongated shape. Its color profile suggests an older stellar population, with a yellowish-orange hue indicative of evolved stars. There is a possible, subtle dust lane that can be seen to the south. It is difficult to discern any spiral arm structure or active star-forming regions. The galaxy appears relatively isolated, showing no obvious signs of tidal interactions or recent mergers.
