The galaxy presents as an elongated, cigar-shaped structure, likely an edge-on spiral or lenticular galaxy. A central bulge region displays a yellowish-orange hue, potentially indicating an older stellar population. The disk exhibits a bluer tint towards the outer edges, possibly reflecting ongoing star formation. While a smooth component dominates, subtle irregularities or features can be distinguished. No prominent spiral arms or a bar structure are discernible. There is no obvious sign of a major merger, but minor tidal disturbances cannot be ruled out due to the limits of image resolution. Overall, it suggests a massive galaxy with moderate star formation.
