The galaxy presents as a lenticular system, characterized by a smooth, elliptical light distribution and an absence of well-defined spiral arms. The central bulge is prominent, displaying a yellowish hue indicative of an older stellar population. The disk component appears relatively thin and elongated, suggesting it is viewed at a significant inclination. There is a noticeable color gradient, with the central regions appearing redder compared to the bluer outer regions of the disk, potentially indicating ongoing star formation at the outskirts. Overall, the galaxy exhibits a relatively smooth and undisturbed morphology, with no obvious signs of recent major merger events, although there may be signs of minor disturbances present. 
