The galaxy presents an elliptical morphology, with a relatively smooth light distribution. The galaxy's color suggests an intermediate age stellar population. There is likely ongoing star formation within the galaxy, although at a low rate. There appears to be a possible ongoing merging event. The overall structure suggests a relatively relaxed system, potentially transitioning from a more dynamically disturbed state. The galaxy's size appears moderate relative to other galaxies. The object could be classified as an early-type spiral galaxy, potentially exhibiting characteristics of an ongoing transformation to a more elliptical form.
