The galaxy presents a generally smooth and elliptical morphology, with a high degree of central concentration. The core exhibits a bright, yellowish hue, suggesting an older stellar population. Moving outwards from the core, the galaxy transitions to a fainter, more diffuse outer region, retaining a largely featureless appearance. There is minimal evidence of spiral arm structures or significant dust lanes visible in this imaging. Subtle color variations exist within the galaxy's structure, hinting at minor differences in stellar populations or dust content across its extent. No prominent signs of tidal interactions or major mergers are readily apparent. Overall, the galaxy appears to be a relatively undisturbed system with a dominant spheroidal component.
