The galaxy presents as a centrally concentrated system with a spheroidal morphology. A bright, yellowish core dominates the structure, suggesting a high concentration of older stellar populations. Fainter bluish hues surround the core, potentially indicating regions of more recent, albeit subdued, star formation within a disk-like component or outer envelope. The galaxy appears largely undisturbed with a smooth overall texture. The light distribution is relatively uniform without obvious spiral arms or significant irregularities. The overall color is muted, trending towards redder wavelengths, consistent with a passively evolving system. There is very little evidence of dust lanes or significant gas content.
