The galaxy appears to be a relatively smooth, elliptical system. Its color is predominantly yellow-orange, suggesting an older stellar population with fewer young, massive stars. The light distribution is centrally concentrated, with a gradual decline in surface brightness outwards. There is little evidence of spiral arms or significant dust lanes. The overall morphology indicates a system that has undergone significant merging in its history, resulting in a fairly homogenous spheroidal shape. There is a potential faint tidal tail on the right side of the galaxy that might have been a result of a previous galaxy interaction.
