The galaxy presents as an elliptical morphology, exhibiting a high degree of central concentration. The light distribution suggests a smooth profile, with a gradual decline in surface brightness from the core outwards. There's a subtle color gradient observed, with the central region appearing more yellow, potentially indicating an older stellar population. The outer regions appear slightly bluer, possibly due to the presence of younger stars or ongoing star formation at a relatively low rate. The overall shape is close to circular, indicating minimal distortion due to interactions. Based on the light profile, it does not exhibit clear spiral arm structures or a distinct disk.
