The galaxy presents as a single, centrally concentrated object with a smooth light distribution, showing little evidence of spiral arms or a distinct disk structure. The galaxy's morphology appears to be elliptical, exhibiting an intermediate roundness. There is a slight elongation, with the major axis oriented approximately northeast-southwest. The central region displays a high surface brightness, indicating a dense concentration of stars. Fainter light extends outwards from the core, gradually decreasing in intensity. There are no clear signs of ongoing mergers or major disturbances in its structure, although some subtle asymmetries in the outer regions cannot be entirely ruled out. The galaxy appears relatively isolated, with no obvious signs of tidal interactions with neighboring galaxies. Colors appear to be redder in the central part of the galaxy.
