The galaxy presents as a concentrated, centrally-brightened object. Its morphology appears largely smooth, exhibiting a generally elliptical shape. The light profile suggests a dominant spheroid component. Some minor disturbances may be present within the galaxy, but do not disturb the round symmetry. The overall colouration is consistent with an older stellar population. There's evidence of a nearby object that appears to be interacting with the galaxy, it is much smaller in size and less luminous.
