The galaxy presents a generally smooth and elliptical morphology. It exhibits a concentrated central bulge that appears quite luminous, indicating a high stellar density. The color profile suggests a predominantly older stellar population, with a yellow-red hue indicative of evolved stars. There is minimal evidence of spiral arms or significant dust lanes. The overall appearance is consistent with an elliptical galaxy, likely a massive system with relatively low current star formation activity. Subtle irregularities in the outer regions may suggest minor gravitational interactions or past mergers. The galaxy's structure appears largely undisturbed, suggesting a stable and relaxed system.
