The galaxy presents as a relatively smooth, elongated structure, exhibiting a color gradient from a more yellow central region to slightly bluer edges. The morphology is largely smooth, with some subtle indications of internal features, possibly faint spiral arms or dust lanes, though these are not sharply defined. The galaxy appears to be lenticular or a tightly wound spiral, seen at an angle. The light distribution suggests an older stellar population dominating the central bulge, while the bluer light in the outer regions indicates more recent star formation, albeit at a modest rate. There is no evidence of ongoing major merger activity.