The galaxy presents as a relatively smooth, elliptical-like structure with a bright central bulge that appears to dominate the overall morphology. The visible light emission suggests a population dominated by older stars, contributing to the galaxy's yellowish-white color. There are indications of a possible disk-like structure, although it's not sharply defined, contributing to the classification as "in between" in shape. A slight asymmetry or disturbance on one side implies there may have been some kind of past interaction, although there is no obvious major merger apparent. The galaxy demonstrates low levels of star formation.
