The galaxy presents as a relatively smooth, elliptical-like structure. It appears to be quite compact with a noticeable central bulge that emits a significant amount of light, suggesting a high concentration of stars. The color profile is predominantly yellow-orange, hinting at an older stellar population with minimal ongoing star formation. There is a slight color gradient, with the central region appearing more yellow. No prominent spiral arms or distinct dust lanes are discernible in this image. There is only a very slight hint of a disk. There does not seem to be signs of any tidal disturbances or ongoing mergers.
