The galaxy presents as a relatively smooth, elliptical or spheroidal structure. It exhibits a centrally concentrated luminosity profile, suggesting a dominant bulge component. The color gradients are subtle, with a slightly bluer halo surrounding a redder core. This implies a radial variation in stellar populations, with younger, bluer stars populating the outer regions and older, redder stars concentrated towards the center. There is no discernible spiral arm structure or prominent dust lanes evident in the image, consistent with a classification towards the early end of the Hubble sequence. The overall symmetry indicates a relaxed morphology, without signs of major tidal disturbances or ongoing mergers. The image suggests moderate star formation activity, based on the subtle blue tint.
