The galaxy presents an elliptical morphology, with a smooth, concentrated light distribution. The galaxy's core exhibits a yellowish hue, suggesting a population of older stars. Moving outward from the core, a diffuse, bluish halo becomes apparent, which could indicate some presence of younger, hotter stars and regions of ongoing star formation, however minimal. There's no clear indication of spiral arms or a prominent disk structure. The galaxy's overall shape is more elongated than circular, with a relatively high degree of smoothness in its stellar distribution. There are no obvious signs of major mergers or tidal disturbances in the immediate vicinity.
