The galaxy presents as an elongated, disk-like structure, viewed nearly edge-on. A prominent bulge is evident, concentrated towards the center of the galaxy. The bulge exhibits a rounded morphology. The disk appears relatively smooth, with a lack of readily discernible spiral arm structures. The color distribution suggests a possible gradient, with the central bulge exhibiting a yellowish-orange hue that may indicate an older stellar population. The outer regions of the disk appear bluer, potentially indicating the presence of younger stars and ongoing star formation. No major merger events or significant disturbances are apparent. Based on the galaxy's characteristics, it is likely a spiral galaxy viewed edge-on.
