The galaxy presents as a smooth, elongated structure with a central bulge exhibiting a yellowish hue, suggesting an older stellar population concentrated in the core. The galaxy's disk, oriented at an angle to our line of sight, displays a subtle gradient in color, transitioning from the yellowish core to a bluer periphery. This color difference implies ongoing star formation in the outer regions. The overall form is cigar-shaped, lacking any readily discernible spiral arms or significant disturbances in its structure. The galaxy appears relatively undisturbed, with no obvious signs of a recent major merger or interaction. 
