The galaxy presents an elliptical morphology, displaying a flattened disk-like structure when observed from our vantage point. A distinct color gradient is visible across the galaxy's body, transitioning from a bluish hue at the periphery to a reddish tone toward the central region. This suggests potential variations in stellar populations, dust content, or redshift across the galactic structure. Further investigation is needed to determine the exact causes of this color variation. There is a hint of some distortions in the disk shape, which could be indicative of possible past interactions with other galaxies. There may also be some minor tidal features present, but these are not clearly defined. The majority of the galaxy's light appears to be concentrated in the central bulge, although the overall light profile seems relatively smooth and integrated.
