The galaxy presents an elliptical morphology, appearing largely featureless and smooth in structure. The central region exhibits a bright, concentrated luminosity that gradually diminishes towards the outer edges. Color gradients are subtle but noticeable, transitioning from a yellowish-white core to a slightly greenish hue in the surrounding areas, indicating a possible mix of stellar populations and dust content. No prominent spiral arms, bars, or signs of recent major mergers are discernible, suggesting a relatively relaxed dynamical state. The overall appearance suggests a galaxy dominated by older stellar populations, consistent with a low rate of on-going star formation.
