The galaxy presents as a relatively smooth, elliptical-like structure. Its overall color profile appears to be dominated by reddish-yellow hues, suggesting an older stellar population with a lower rate of ongoing star formation. The central region exhibits a higher surface brightness, indicative of a concentrated galactic nucleus. There's a slight elongation to the galaxy's shape, but it largely approximates a spheroid. No prominent spiral arms or significant dust lanes are readily discernible in the image, reinforcing the inference of a smooth, evolved system. There is no immediately observable evidence of strong tidal interactions or recent merger events, though minor disturbances cannot be ruled out based solely on this image.
