The galaxy presents as a relatively smooth, disk-shaped system observed nearly edge-on. A central bulge is apparent, exhibiting a yellowish-white hue suggestive of an older stellar population. Extending outwards from the bulge, a faint disk is visible. The disk displays a bluer color, hinting at ongoing star formation. The morphology suggests a possible spiral galaxy viewed at high inclination. There may be some minor disturbances indicating a possible gravitational interaction. Based on the observed color gradient, the galaxy appears to have a moderate mass and star formation rate.
