The galaxy presents as a moderately bright, relatively smooth, and centrally concentrated object. Its overall shape is somewhat elliptical, though not perfectly round, appearing slightly elongated. No distinct spiral arms or bar structures are discernible in the image. There are hints of some internal structure; the central region appears slightly brighter and more uniform in color, possibly indicating an older stellar population or bulge component. The outer regions seem to fade gradually, showing a subtle color gradient that appears redder towards the periphery. There are no obvious signs of significant ongoing star formation activity based on the color or morphology visible in this image. No significant tidal tails or other signs of recent major merger events are visible, although there may be some minor disturbances within the galactic disk. 
