The galaxy presents as an elliptical morphology, appearing mostly smooth with a high degree of central concentration. The color profile indicates an older stellar population, with redder hues dominating, especially within the central bulge region. There is a subtle color gradient from the core to the outer regions, suggesting a possible variation in stellar ages or metallicity, with bluer colors possibly indicating more recent star formation in the outer regions, although this is not a dominant feature. No distinct spiral arm structures or dust lanes are visible. The galaxy appears relatively undisturbed, showing no significant signs of ongoing mergers or tidal interactions.
