The galaxy appears as a relatively smooth, elliptical structure. The central region exhibits a concentrated, bright core. Fainter light extends outward from the core in a roughly circular distribution. There is a slight elongation, suggesting it is not perfectly spherical. Some minor disturbances are present, which could be due to a past or ongoing minor interaction or merger. The overall color profile indicates an older stellar population, with a predominantly redder hue, suggesting a reduced rate of star formation.
