The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that is luminous and gradually diffuses outwards to a fainter halo. The overall shape appears nearly circular. There's a subtle color gradient from the core to the outer regions, with the central region appearing bluer and the outer regions redder, suggesting a potential age difference in the stellar populations, with the core having younger stars. The lack of prominent dust lanes or spiral arms suggests a relatively quiescent galaxy with little ongoing star formation. There is no evidence of significant tidal disturbances or ongoing merging events within the immediate field of view, however, there may be very minor disturbances nearby. The galaxy is a fairly compact galaxy.
