The galaxy presents as a largely smooth, elliptical-like structure with a concentrated central bulge. The light is more yellow at the center and grades to a slightly more reddish hue toward the outer edges. It is largely featureless with no evident spiral arms or significant dust lanes visible. There might be a very slight elongation, but it looks generally round. The overall structure indicates an older stellar population, with minimal current star formation activity. There is no visible evidence of any major ongoing merger event, but minor distortions cannot be ruled out completely at this resolution.
