The galaxy presents as a centrally concentrated object with a smooth overall morphology. It is characterized by a dominant yellowish hue in its central region, which gradually transitions to a redder color profile extending towards the outer regions. A slight asymmetry in the outer regions is noted, with a possible faint tidal feature or minor disturbance observable on one side. There is little evidence of resolved star formation regions or spiral arm structures within the galaxy's visible components. The observed color gradients suggest a declining star formation rate in the galaxy.
