The galaxy presents as a somewhat elongated, lenticular-like structure. The central bulge exhibits a bright, concentrated luminosity, indicative of a significant population of older stars. Diffuse, outer regions suggest a disk, however, there is a lack of well-defined spiral arms. Asymmetrical features suggest a tidal interaction is present. These features could possibly be from the small galaxy companion located nearby. There does not appear to be prominent dust lanes within the primary galactic body based on the lack of reddening in the bulge. Overall, this galaxy displays characteristics of evolved, relatively quiescent system, possibly undergoing interaction with a smaller companion.
