The galaxy presents as a smooth, elliptical structure with a noticeable radial color gradient. The central region appears more concentrated and exhibits a warmer, reddish hue, suggesting an older stellar population or dust obscuration. Moving outwards from the core, the color shifts toward a bluer tint, hinting at the presence of younger stars and possibly ongoing star formation within the extended disk or halo. The galaxy is elongated with an intermediate axis ratio, appearing neither perfectly spherical nor highly flattened. There is no obvious evidence of spiral arms or a prominent central bar. The overall morphology suggests a quiescent galaxy, lacking significant signs of recent major mergers or strong tidal interactions, although some minor asymmetries or disturbances cannot be ruled out at this resolution. The estimated size indicates a substantial galactic mass.
