The galaxy presents as a smooth, elongated object, appearing cigar-shaped in morphology. There is a noticeable color gradient, with the central region exhibiting a yellowish-orange hue, possibly indicating an older stellar population. The outer regions are a pale bluish color, which may suggest some level of ongoing star formation. No distinct spiral arms or bar structures are readily apparent. The overall light distribution appears relatively even and undisturbed, indicating the galaxy is likely not undergoing a major merger event. Based on these observations, it can be tentatively classified as an elliptical galaxy or a lenticular galaxy viewed nearly edge-on.
