The galaxy presents as a single, relatively smooth object. The core appears very bright, gradually decreasing in brightness as one moves outward toward the edges. It has an elliptical, somewhat circular, appearance but is not perfectly round. There is no strong evidence of spiral arms or a disk-like structure. Instead, the light is evenly distributed. It exhibits a slight blue tint, suggesting the presence of some ongoing, but not extreme, star formation. There is no sign of ongoing or recent major merger activity. The overall morphology suggests a galaxy with a large stellar mass.
