The galaxy appears as a relatively smooth, centrally concentrated object. Its overall shape is somewhere between round and elongated, with only a slight deviation from a circular morphology. There is no strong evidence of spiral arm structure or a prominent disk component. The galaxy displays a color gradient, with a bluer hue at the center. This bluer color may indicate the presence of younger, hotter stars in the galaxy's core, perhaps caused by a more recent burst of star formation. There appears to be little to no dust obscuration visible in this image. The galaxy does not appear to be undergoing a major merger, though there is a chance that there may be minor disturbances visible in the future with more detailed observations.
