The galaxy presents as a relatively smooth, elliptical structure, with a concentrated central bulge. The color profile suggests an older stellar population, dominated by redder wavelengths, particularly within the core. There's a subtle gradient outward, with the outer regions appearing marginally bluer than the nucleus, potentially indicating some ongoing, albeit limited, star formation in the disk or halo. No distinct spiral arms or bar features are discernible. The overall morphology suggests a galaxy that is either undergoing a quiescent phase of evolution or is already a well-established elliptical system. There are no obvious signs of major disturbances or interactions with other galaxies. The shape is moderately elongated, not perfectly spherical, but not highly flattened either.
