The galaxy presents as a moderately inclined elliptical or lenticular system, exhibiting a smooth, diffuse light profile characteristic of an older stellar population. The galaxy's overall color appears somewhat blue, potentially indicating the presence of a modest population of younger stars. There is a slight elongation observed, with the major axis oriented approximately Northwest to Southeast. No distinct spiral arms or dust lanes are discernible within the galaxy's structure. The galaxy appears largely undisturbed, showing no signs of major mergers or tidal interactions.
