The galaxy presents an overall elliptical morphology, appearing somewhat elongated in shape. Its light profile suggests a smooth structure with a high degree of central concentration, indicative of a large central bulge component. The color gradients suggest a possible radial variation in stellar populations, with the central region appearing more yellow, potentially signifying older stellar populations compared to the outer regions which have subtle blue tones, which may indicate more recent star formation. There is no distinct spiral arm structure visible, and no significant signs of active galactic nuclei or major disturbances from interactions with other galaxies. There may be very minor disturbances, but they are not very visible. Overall the galaxy is most likely an elliptical galaxy.
