The galaxy presents a relatively smooth and centrally concentrated morphology. It appears elliptical in shape, with a noticeable flattening. There is a distinct, bright core, suggesting a high concentration of stars in the galactic nucleus. The surrounding halo exhibits a more diffuse and fainter luminosity profile, extending further from the center. The galaxy exhibits a subtle color gradient, transitioning from a slightly reddish hue in the central region to a bluer tint in the outer regions. This implies a potential difference in stellar populations, with older, redder stars concentrated towards the core and younger, bluer stars populating the outer disk. There are no apparent spiral arm structures or dust lanes visible in this image. The overall appearance suggests a mature galaxy with a relatively quiescent star formation rate.
