The galaxy presents as a centrally concentrated, elliptical-like structure. Its core exhibits a bright, yellowish hue, indicative of an older stellar population. Moving outward from the nucleus, there is a subtle transition to a more diffuse halo. The halo region shows hints of a slightly bluer color compared to the core, which may suggest the presence of a younger stellar population, although it appears to be overall quiescent. There is no strong evidence of spiral arm structures or significant dust lanes. The overall morphology suggests a relatively smooth, evolved system, with possible, but not apparent, minor disturbances.
