The galaxy presents a largely smooth, elliptical morphology. It appears as a centrally concentrated object with a radial gradient in luminosity, brightest at the core and fading towards the edges. The shape is roughly round but deviates slightly, not appearing perfectly circular. There are some hints of disturbed features. The overall color profile suggests a mature stellar population, as redder hues are visible, particularly towards the central region. However, there is evidence of some star formation, with some bluer regions present, most likely concentrated in the outer areas. The galaxy does not present a clear spiral arm structure nor a prominent disk component. There is no distinct dust lane visible within the galaxy. No major merger is immediately apparent; however, subtle asymmetries and slight irregularities in the outer halo suggest possible minor interactions or past mergers.
