The galaxy exhibits a somewhat elliptical morphology, appearing more "in-between" round and elongated than distinctly circular. The overall light distribution suggests a relatively smooth profile, yet hints of internal structure are apparent. A subtle disk-like component might be present, although the bulge appears dominant. There is some evidence of possible disturbance with some irregular features. The galaxy presents with a blue hue, indicative of some ongoing star formation, although at a relatively low rate. The galaxy is moderately sized.
