This galaxy exhibits a generally smooth morphology, appearing elongated and cigar-shaped. Its color gradient suggests a more pronounced concentration of older stellar populations towards the central regions, with a yellowish hue dominating the core. The outer regions present a bluer tint, possibly indicating the presence of younger stars or ongoing star formation, albeit at a relatively low rate. There is no clear evidence of spiral arm structures or a prominent central bulge. The overall structure implies that this galaxy is an elliptical or lenticular galaxy viewed at a significant angle, with a minor chance of a merger event. The lack of strong features, in conjunction with its color profile, implies a relatively quiescent star formation history.