The galaxy appears to be a relatively smooth, elliptical galaxy with a slightly elongated morphology. The color profile shows a predominantly uniform distribution across the galaxy, with a concentration of light towards the center. There's a very slight gradient towards bluer colors at the periphery, suggesting the presence of some younger stellar populations, but the overall color indicates an older stellar population dominates. The galaxy exhibits minimal visible structure, lacking prominent spiral arms or a distinct disk component. There's no immediate evidence of major mergers or tidal disturbances. The central region seems to be brighter than the outer regions, potentially indicating a more concentrated stellar density. Overall, the galaxy appears to be a relatively evolved system.
