The galaxy presents as a relatively bright, moderately sized object. Its morphology appears to be a disk galaxy viewed at a significant inclination. While a bulge is not particularly prominent in the optical, a faint central concentration of light is observable. The disk itself exhibits subtle color variations, suggestive of active star formation regions. There is also evidence of minor disturbances, which could indicate gravitational interactions. The galaxy is classified as smooth or having features. The smoothness fraction is high, suggesting no major distortions. There is a slight cigar shape to it, but it is mainly an in-between shape. The galaxy is likely not undergoing a major merger, but shows minor disturbances.
