The galaxy appears as a centrally concentrated object, characterized by a smooth light distribution. Its overall morphology suggests an elliptical or lenticular galaxy type, exhibiting a generally rounded form with a slight deviation from perfect circularity. There is no discernible spiral arm structure or evidence of significant dust lanes within this galaxy.

The galaxy's color is predominantly yellow-orange, indicative of a stellar population dominated by older, cooler stars. The presence of such a red color suggests relatively low current star formation activity, and a likely population of evolved stars. The color gradient appears fairly uniform across the galaxy, with perhaps a slightly bluer tinge in the very central region.

There's no strong evidence of any major ongoing merger events or significant tidal disturbances affecting its morphology. The outskirts of the galaxy appear to gradually fade into the background, with no sharp edges or breaks in its stellar halo.
