The galaxy presents as an elliptical morphology, exhibiting a high degree of smoothness. The galaxy displays a centrally concentrated luminosity profile that diminishes gradually towards the outer regions. Color gradients are apparent, with the core exhibiting a yellower, possibly redder, hue which suggests a potentially older stellar population. The overall symmetry is high, showing little to no evidence of significant disturbances, such as tidal tails or asymmetries. There is no clear indication of spiral arm structures or a prominent disk from this visual data. The galaxy appears relatively isolated.
