The galaxy presents as a largely featureless elliptical system, exhibiting a smooth and concentrated light profile. The central region appears very bright, gradually fading into the outer regions. The overall shape is elongated, appearing somewhere between round and cigar-shaped, suggesting a possible E4-E5 classification on the Hubble sequence. There is no visible evidence of spiral arms or a prominent disk structure. Additionally, there are no obvious signs of any significant ongoing or recent merger events, major disturbances, or tidal features. The color is primarily bluish white, suggesting the presence of intermediate to old stellar populations. Overall, the galaxy's appearance is indicative of an evolved system with minimal ongoing star formation.
