This galaxy presents a largely smooth morphology, appearing as a concentrated, somewhat elliptical form. The central region exhibits a brighter, yellowish hue, suggesting an older stellar population. Fainter, bluish extensions surround this central bulge, possibly indicative of ongoing star formation. There is a slight hint of disturbances or asymmetries in the outer regions, perhaps evidence of minor gravitational interactions. The overall structure suggests a system dominated by an older, spheroidal component with some residual star formation in the outer regions.
