The galaxy presents as a spiral type, observed at a near face-on orientation. Two distinct spiral arms are visible, exhibiting a moderate winding pattern. The arms originate from a prominent central bulge. The bulge appears orange in color which suggests an older stellar population compared to the disk. A faint bar-like structure appears to extend through the center of the bulge, with medium strength. The disk exhibits a mottled texture, implying ongoing star formation, with regions of younger, bluer stars distributed throughout the spiral arms. There is no clear indication of a major ongoing merger or significant tidal disruption. Overall, the galaxy displays a fairly regular spiral structure with a moderate bulge and signs of active star formation within its spiral arms.
