The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated light profile. There is a high degree of central concentration. The galaxy's overall color appears redder in the central region, transitioning to bluer hues in the outer regions. This color gradient suggests older stellar populations are dominant in the core, while younger, hotter stars are more prevalent in the outer disk. There is no prominent spiral arm structure or any other obvious sign of significant ongoing major mergers, interactions, or star formation. The object is significantly elongated, though no obvious bar or disk structure is visible.
