The galaxy presents as a relatively compact object with an apparent smoothness of structure. Its morphology is approximately elliptical, tending toward a circular shape. The light is concentrated toward the core, gradually decreasing in intensity towards the outer edges. The galaxy's color profile indicates bluer wavelengths in the central part, suggesting the presence of hotter, younger stars or active galactic nuclei processes. There is also the possibility of some minor irregularity in the galaxy's outer regions, which may be indicative of a past interaction or minor disturbance. No clear indications of spiral arm structure or a prominent disk component are visible in the image. Overall, the galaxy appears to be largely undisturbed, with a dominant smooth spheroid shape.
