The galaxy presents as an edge-on spiral or lenticular system, characterized by a distinct central bulge that appears roughly spheroidal and displays a yellowish-white color, suggesting an older stellar population. The disk is viewed nearly edge-on. The disk shows a noticeable blue tint, implying the presence of younger, hotter stars and recent star formation activity. The presence of dust lanes are suspected within the disk. The disk is relatively smooth, with no obvious major distortions or tidal features, suggesting it has not undergone a major merger recently. The overall morphology is relatively undisturbed. The galaxy exhibits a measurable redshift, indicating its distance and recessional velocity.
