The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a high concentration of light, appearing bright and nearly spherical. Moving outward from the core, the light gradually diffuses, maintaining a generally elliptical shape. There is only a slight deviation from perfect ellipticity. No distinct spiral arms, bars, or prominent dust lanes are discernible in the image. The color gradient transitions subtly from a yellowish-white at the core to a faint bluish hue in the outer regions, suggesting a population of older stars concentrated towards the center, with younger, bluer stars potentially existing in the outer extents. There is no clear indication of ongoing major merger activity, though subtle asymmetries might suggest minor disturbances. The overall impression is that of a relatively evolved, quiescent system.
