The galaxy presents as an edge-on disk galaxy. A prominent central bulge with a yellowish hue suggests an older stellar population concentrated towards the core. The disk component, extending laterally from the bulge, exhibits a bluer color gradient indicating ongoing star formation and a younger stellar population. The disk appears relatively smooth, lacking well-defined spiral arm structures. The high disk inclination obscures detailed morphological features. There is no evidence of major mergers, strong tidal features, or significant morphological disturbances. Overall, this galaxy appears to be a relatively undisturbed, actively star-forming disk galaxy viewed edge-on.
