The galaxy presents as a somewhat elliptical structure, appearing largely smooth in texture with a concentrated central bulge. The color profile suggests a mixed stellar population. The central region exhibits a yellowish hue, possibly indicating older, cooler stars. Moving outward from the core, a greenish tint is observed, potentially indicating the presence of some ongoing, albeit low, star formation. The galaxy's overall structure seems undisturbed, displaying no obvious signs of major mergers or significant tidal interactions. It appears relatively isolated, maintaining a fairly uniform density profile from its core to its observed edges.
