The galaxy presents a primarily smooth morphology, with a hint of subtle features potentially indicative of a disk or spiral structure, although this is not definitive from the image. The overall shape is somewhere between round and in between round and elliptical, showing some degree of ellipticity. There are no strong indications of ongoing major merging events; however, subtle disturbances could be present. The color gradient suggests a redder core region that gradually transitions to bluer outskirts. This color difference might indicate a population gradient within the galaxy, with older, redder stars concentrated towards the center and younger, bluer stars towards the periphery. It appears to be a relatively massive galaxy with intermediate star formation activity based on its luminosity.
