The galaxy appears to be a relatively smooth and symmetrical system, displaying characteristics that suggest an elliptical morphology. It presents a centrally concentrated luminosity profile, with a brighter core gradually fading towards its outer regions. While some subtle features or irregularities can be discerned, the overall impression is one of a well-defined, single object without pronounced spiral arms or a distinct disk-like structure. The color gradient indicates a likely population of older stars with reduced star formation activity. The galaxy's light seems to be slightly distorted, suggesting the possibility of a previous minor disturbance, however this effect is not strongly pronounced.
