The galaxy presents as an elliptical morphology, with a smooth, diffuse light distribution indicating a lack of prominent spiral arms or a distinct disk. The central bulge exhibits a bright, concentrated luminosity, suggesting a high density of stars. The galaxy appears slightly elongated along one axis, hinting at a moderate degree of ellipticity, but it is not highly flattened. There is evidence of color variation across the galaxy, with a bluer hue along the outer edges, possibly indicating younger stellar populations or ongoing star formation in these regions, while the central regions appear redder, likely composed of older, redder stars. There is no visual evidence of a major merger event, although some minor disturbances or faint tidal features cannot be ruled out based on this image alone.
