The galaxy presents as a smooth, elongated structure, likely a spiral galaxy seen nearly edge-on. A bright central bulge is observed, with a yellowish hue, suggesting an older stellar population. Faint, diffuse extensions emanate from either side of the bulge along the major axis, indicating the presence of a disk. These extensions exhibit bluer tones, possibly indicative of younger stars and ongoing star formation. The overall morphology suggests an undisturbed system with no obvious signs of recent major merger activity, although minor asymmetries may be present. The light distribution is centrally concentrated, fading gradually towards the outer regions of the galaxy.
