The galaxy presents a largely smooth morphology, with a generally elliptical profile. The central region exhibits a high surface brightness, appearing as a concentrated and intensely luminous core. The light gradually diffuses outwards from the core, forming an extended halo characterized by a lower surface brightness. There is only a slight suggestion of any disc-like or spiral features. The overall color appears relatively uniform. There is no apparent evidence of any major ongoing merger activity or tidal disturbances. The galaxy appears to be an early-type system dominated by an older stellar population. 
