This galaxy appears to be a relatively smooth elliptical, presenting a bright, concentrated central bulge. The light distribution is fairly even, with no discernible spiral arms or prominent dust lanes. The galaxy is somewhat flattened, appearing nearly circular on the sky with a slight ellipticity. A very slight color gradient is seen, appearing bluer towards its outer edges, indicating a possible difference in stellar population or age between the core and periphery. There are no visible signs of any major ongoing merging events or tidal disturbances in the system. Overall, the galaxy presents an undisturbed and relatively evolved morphology.
