The galaxy presents as a fairly smooth, centrally concentrated object. It exhibits a largely elliptical morphology, appearing mostly round, with some deviation. The galaxy displays a noticeable color gradient, transitioning from a bluer hue in its outer regions to a redder, more yellowish core, which may suggest a difference in stellar population or dust content. There is no clear evidence of spiral arms or a prominent disk structure. Similarly, there are no obvious signs of recent major merger activity, although subtle disturbances cannot be ruled out. The overall texture of the galaxy appears smooth, potentially indicating an older stellar population.
