The galaxy presents a relatively smooth, rounded morphology. There is a suggestion of a disk-like structure, but it's not highly prominent. The light distribution is concentrated towards the center, indicating a bulge or core region. The galaxy exhibits a blue hue, which is typical of star-forming galaxies or galaxies with a significant population of young, hot stars. However, there is minimal visible indication of recent major mergers or significant disturbances, suggesting a relatively stable, evolved system. The galaxy does not exhibit clear spiral arm structure in this image. It has an apparent size of a small angular extent.
