This galaxy exhibits a somewhat elliptical morphology, appearing relatively smooth in structure. The central region is bright and concentrated, potentially indicating the presence of a significant bulge or active galactic nucleus. The overall color of the galaxy appears blueish-green, which could suggest the presence of ongoing star formation. Faint indications of disturbances in the outer regions may exist. It does not appear to be undergoing a major merger, but there is a possibility of minor disturbances due to tidal interactions. A significant portion of the light in this image is contributed by light in the green and blue portions of the spectrum, with less light in the red portions of the spectrum. This may indicate a population of younger stars.
