The galaxy presents a generally smooth and elliptical morphology, with a dominant central bulge region exhibiting a yellowish hue, suggesting an older stellar population. There is a subtle indication of a disk structure. A bluer, less luminous region is observed, possibly indicating a region of ongoing star formation. Based on the morphology, it is likely an elliptical galaxy that may be undergoing a minor merger event. The lack of strong spiral arms or significant dust lanes further supports an elliptical classification.