The galaxy presents a largely smooth and rounded morphology. It appears to be an elliptical galaxy with a concentrated central bulge that graduates to more diffuse, yet still smooth outer regions. There is a slight elongation to its shape, but it is generally round. Evidence of a disk or spiral arms is absent. No major disturbances or merging events are immediately apparent, though some minor asymmetry or faint features could indicate past interaction. The color profile suggests a population of older stars, resulting in a reddish hue. There is a lack of distinct features.