The galaxy presents as a single, centrally concentrated object. It appears elliptical, with a smooth, diffuse light distribution. The core exhibits a bright, yellowish hue, suggesting an older stellar population. The overall shape is quite round and undisturbed, showing no obvious signs of spiral arms or a distinct disk. There's no significant presence of blue light or dust lanes visible in this particular observation, indicating a low ongoing star formation rate. There are no obvious signs of a major ongoing merger event. The galaxy shows as being generally smooth and appears to have a round shape, which could mean that the bulge dominates the galactic structure.
