The galaxy appears as a somewhat elliptical or disk-like system with a centrally concentrated bulge. The color gradient suggests a population of older stars dominating the core, exhibiting a yellow-orange hue. Fainter, slightly bluer, features seem to extend outward from the central region, hinting at the presence of some younger stars or regions of ongoing star formation in the outer disk. Overall, the galaxy does not show strong signs of recent major merger activity or significant tidal disturbance.
