The galaxy presents a moderately inclined disk structure. A prominent central bulge, exhibiting a yellowish-orange hue, dominates the core region. Extending outwards from the bulge is a fainter, yet discernible, disk. The disk appears relatively smooth. Within the disk plane, observations reveal potential spiral arm fragments. The color gradient suggests ongoing, albeit potentially subdued, star formation within the disk, specifically concentrated in the aforementioned fragmented arm structures. The galaxy appears to have no major mergers or interactions with other galaxies. The smooth features and lack of major disturbances indicate it has reached a stable morphological configuration.
