The galaxy presents a largely elliptical morphology, with a high degree of central concentration. Its overall appearance is smooth and featureless, lacking any discernible spiral arms or distinct structures. The luminosity profile appears to decrease monotonically from the core outwards. The color index shows a redder central region with bluer outskirts, suggesting potential differences in stellar populations or dust content between these areas. There is no indication of any major ongoing merging activity or significant tidal disturbances. The galaxy is likely a relatively massive system, possibly on the higher end of the mass distribution of observed galaxies. Star formation activity appears to be minimal.
