The galaxy presents as a largely featureless, elliptical morphology. It exhibits a smooth, symmetrical light distribution, with a centrally concentrated and highly luminous core. The radial profile of the galaxy indicates a gradual decrease in brightness from the center outwards, suggesting a high degree of stellar population homogeneity. There is no apparent spiral arm structure or dust lane obscuration discernible in this image. Faint and diffuse light extends outwards, indicating a moderate-sized halo. There is no evidence of any tidal features or interactions with neighboring galaxies.
