The galaxy appears to be a relatively smooth, elliptical-like structure, approximately circular in shape. The light distribution is concentrated towards the center, fading gradually outwards without any distinct features like spiral arms or a prominent disk. The core exhibits a brighter intensity, suggesting a higher concentration of stars or a possible active galactic nucleus, though this cannot be confirmed from the image alone. No significant tidal tails or distortions are discernible, indicating that the galaxy is not currently undergoing a major merging event. A very subtle asymmetry might be present in the outer regions, requiring further investigation with higher resolution data. Overall, the galaxy presents as a well-defined, quiescent system.
