The galaxy presents as a centrally concentrated object with a generally smooth appearance, exhibiting a near-circular morphology. The core exhibits a bright, yellowish-white hue. A subtle color gradient is observed, transitioning to a redder and dimmer halo. No distinct spiral arm structures or prominent dust lanes are discernible. The overall structure suggests a relatively evolved system, potentially an elliptical galaxy or a lenticular galaxy viewed close to face-on. Minimal signs of tidal interactions or ongoing mergers are evident. Based on the color profile, star formation appears suppressed or negligible.
