The galaxy presents as a relatively compact, elliptical-like system. It exhibits a smooth, centrally concentrated luminosity profile, with a bright yellowish core that gradually fades into a less luminous halo. There is no apparent spiral arm structure or prominent dust lanes visible. The overall shape is nearly circular, with only a slight elongation. There is no sign of a tidal tail or merger event. The galaxy appears quiescent with low levels of star formation, with the core composed of older stellar populations, emitting light towards the redder end of the spectrum.
