The observed galaxy presents as an edge-on spiral, exhibiting a distinct disk-like structure. The galaxy's central bulge appears prominent and elongated along the major axis of the disk. The bulge displays a smooth, rounded morphology, with an overall yellow-orange hue. The disk component is relatively thin and exhibits hints of dust lanes, though these features are not sharply defined. The overall color gradient suggests a stellar population primarily composed of older stars. There are no discernible signs of a recent major merger event, although there are hints of a minor disturbance, possibly from an ongoing interaction. The luminosity is moderate, implying a medium-sized galaxy. There is no distinct spiral arm structure visible. The galaxy does not appear to be actively undergoing a major starburst.
