This galaxy presents as an elongated, cigar-shaped object. It appears to be an edge-on spiral galaxy, given its axial symmetry and high aspect ratio. There is a noticeable color gradient from the core outwards, with a concentrated, brighter yellowish center. This likely indicates an older stellar population dominating the core. The outer regions display fainter, bluer hues. This suggests the presence of younger, hotter stars within the galactic disk. The smooth appearance indicates it is likely an earlier type spiral galaxy. There is no indication of a strong tidal interaction or major merger event disrupting its morphology. It exhibits an unperturbed disk structure.
