The galaxy presents as a relatively small, yet luminous, spiral galaxy, observed at a significant inclination. It appears to have a bright, concentrated central bulge, from which spiral arms emanate. The disk component demonstrates noticeable dust lanes obscuring some of the starlight, particularly on the near side of the disk. The spiral arms are somewhat tightly wound, contributing to the galaxy's overall compact appearance. There is evidence of active star formation within the arms, indicated by the presence of blue regions, but this appears to be fairly subdued. The smoothness fraction indicates it has some features like a smooth galaxy, but not completely smooth. There is no strong evidence of any major merger events or significant tidal disturbances. The overall morphology suggests a galaxy undergoing relatively quiescent evolution.
