The galaxy presents as a concentrated, elliptical morphology. It is characterized by a smooth light profile with a bright, yellow-white core, indicating a likely high concentration of older stellar populations. The overall structure appears largely spheroidal, with only subtle color variations suggesting minimal recent star formation. The shape is generally round. The galaxy lacks any obvious signs of spiral arms or a prominent disk component. There is no evidence of major mergers or tidal disturbances in the surrounding region. 
