The galaxy exhibits a distinct, centrally concentrated bulge region, appearing smooth and luminous. Surrounding this bulge is a disk component, which, while less bright, is clearly visible. The disk appears relatively inclined to our line of sight, as it has an elliptical shape. There is a hint of spiral structure within the disk, though it is not sharply defined, and appears more flocculent. There are no significant dust lanes immediately visible in the disk. Overall, the light distribution appears to be relatively smooth and symmetrical, suggesting a mature system that may not have had a recent major merger event, though minor disturbances cannot be ruled out. The colours are consistent with a population of older stars in the bulge and disk, with only slightly bluer light indicating ongoing star formation.
