The galaxy presents a generally smooth, somewhat rounded morphology. There is little indication of a strong spiral structure or a dominant disk. The light distribution appears relatively even across the body of the galaxy, which implies either an elliptical galaxy shape or a face-on spiral galaxy with very tightly wound arms. There is a suggestion of minor disturbances in the galaxy's morphology, possibly due to a past or ongoing minor merger event. The color gradients present suggest ongoing or recent star formation, particularly concentrated in the galaxy's core. The galaxy appears to have a relatively high mass and high rate of star formation, with a corresponding relatively low specific star formation rate.
