The galaxy appears to be a spiral galaxy with a prominent, moderately sized bulge. There is evidence of spiral arms, although they are not sharply defined. The galaxy shows a slight inclination, but is not viewed edge-on. The central bulge exhibits a yellow-orange hue, indicative of an older stellar population. The spiral arms display a bluer color, suggesting ongoing star formation. No significant mergers or major disturbances are apparent. The overall morphology is typical of a spiral galaxy with a fairly well-defined disk component. There is no dominant bar structure detected, although it is possible a weak bar exists. The galaxy displays a smooth appearance, but is not completely smooth and featureless.
