The galaxy exhibits an elliptical morphology, appearing relatively smooth and featureless. It possesses a slightly elongated shape, with a significant axis ratio, but not so much as to classify it as highly flattened. The central region displays a concentrated luminosity, suggesting a possible bulge component. The color gradient shifts from a yellow/orange hue in the center to a slightly bluer hue towards the outer edges. This color variation could indicate differing stellar populations, with older, redder stars concentrated in the bulge and younger, bluer stars in the outer disk or halo. There's no readily apparent spiral arm structure or dust lane visible in the image, implying that the galaxy may be an early-type galaxy with little current star formation. Faint diffuse light extends outwards, defining the galaxy's halo region. There appears to be no signs of a major ongoing merger or tidal disturbances.
