The galaxy presents a largely smooth morphology. The light distribution appears centrally concentrated with a gradual decrease in intensity towards the outer regions, which lack distinct spiral arm structures or a prominent disk. It exhibits a nearly circular shape. The color profile suggests an older stellar population, with a yellowish-orange hue dominating the central region, gradually shifting towards a redder tone in the outskirts. There is no evidence of ongoing major merging activity, although subtle asymmetries or irregularities might indicate minor disturbances or interactions with nearby objects. The overall structure indicates a system approaching an elliptical morphology with an absence of significant star formation.
