The galaxy presents as a flattened, disk-like structure, oriented nearly edge-on relative to the observer. The central region exhibits a concentration of light, suggesting a bulge component, possibly with a spheroidal or elliptical morphology. The bulge appears to be relatively smooth and gradually fades into the disk. The disk itself shows a faint, diffuse structure. There is a distinct dust lane feature bisecting the galaxy, most likely obscuring much of the galaxy. Based on the light profile, the galaxy's radial light distribution is well fit by a Sersic profile. There does not appear to be evidence of any significant ongoing major merger activity or strong tidal features.
