The galaxy appears as a somewhat elongated, lenticular-like structure. Its light is generally uniform with a very slight central bulge. The disk of the galaxy appears mostly smooth. Although there is no central point-like source, it does appear the galaxy is much brighter in the center than the edges, indicating a possible supermassive black hole. There are no well-defined spiral arms and it does not seem to be interacting with any nearby galaxies. The color index suggests a population of older stars. This is consistent with a relatively quiescent galaxy.
