This galaxy presents as an edge-on spiral, exhibiting a flattened, elongated morphology. There is a noticeable central bulge that appears yellowish-orange, possibly indicating an older stellar population. The disk is prominent with a distinct dust lane, which causes some obscuration, tracing along the equatorial plane of the galaxy. Fainter, diffuse blue regions are observed extending from the disk, which may indicate areas of more recent star formation. Overall, the galaxy seems relatively undisturbed, with no signs of any major mergers or interactions. The galaxy displays a smooth appearance, with some disk features. The color profile suggests a range of stellar populations and star formation activity.
