The galaxy presents as a generally smooth and rounded object. There appears to be a central concentration of light that fades gradually outwards towards the edges. A subtle elongation is observed, suggesting a disk shape viewed at an oblique angle. The color profile indicates a higher concentration of older stars due to the redder hue. No significant signs of recent mergers or tidal disturbances are evident, as the structure appears relatively undisturbed. There may be low-level star formation activity but it is not readily apparent in this image.
