The galaxy presents as a centrally concentrated system with a smooth light distribution. It appears elliptical in shape, exhibiting a high degree of roundness. There is a noticeable color gradient, shifting from a yellowish-white core to a redder hue in the outer regions. No distinct spiral arms, bar structure, or prominent dust lanes are observed. The galaxy appears largely undisturbed, showing no obvious signs of tidal features, mergers, or significant interactions with neighboring galaxies. Its morphology indicates a lack of significant ongoing star formation, instead it appears to consist of an aging stellar population.
