The galaxy appears as a centrally concentrated spheroid with a smooth morphology. The color profile suggests an older stellar population, with a dominant yellowish-orange hue at the core that graduates into more greenish colorations in the outer regions. The object's central region exhibits high luminosity, declining outwards, indicating a high degree of concentration. There is no obvious spiral structure or prominent disk. There is also no strong evidence for any ongoing merger activity or tidal disturbance affecting its structure in this image. The overall shape is somewhere between round and elliptical, trending toward a smooth, relaxed appearance. Overall, it resembles a typical elliptical galaxy, with no ongoing star formation.
