The galaxy presents as an elliptical or lenticular system, showing a predominantly smooth, symmetrical structure. The light distribution suggests an older stellar population, exhibiting a yellow-orange hue, with a bright central bulge and a surrounding halo. The core of the galaxy appears relatively concentrated and displays no obvious signs of recent major mergers or significant tidal disturbances, though minor disturbances cannot be ruled out. There appears to be a second, more distorted system in the same line of sight which may or may not be interacting. Overall, the system lacks prominent spiral arms or dust lanes, implying a relatively quiescent star formation history.
