The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits a slightly elliptical morphology, but is mostly in between round and elliptical. A bright, possibly yellowish core is visible, suggesting a concentration of older stars and possibly a supermassive black hole. Fainter, bluish, extended regions are apparent around the central core, indicating the presence of younger stars. No distinct spiral arm structure is immediately evident. There may be some minor disturbances in the galaxy's symmetry, perhaps related to a recent minor merger. Overall, this galaxy shows properties of an elliptical galaxy with recent star formation.
