The galaxy appears as a relatively smooth, elliptical-like structure, exhibiting a fairly symmetrical and round morphology. It lacks any prominent spiral arms or bar features. The light distribution is concentrated towards the center, with a gradual decrease in intensity outwards. There is a slight bluish hue suggesting ongoing, but weak, star formation. No signs of major mergers or significant tidal disturbances are apparent in this image, although there may be some minor interaction at play given the faint asymmetry. The galaxy appears to be isolated in this field of view.
