The galaxy presents as an elliptical morphology, exhibiting a high degree of smoothness in its light distribution. The central region displays a concentrated, bright core, suggesting a significant density of stars. A faint, extended halo surrounds the core, gradually fading into the background sky. The overall color appears slightly reddish or yellow, hinting at a relatively older stellar population. There are no prominent spiral arms or dust lanes visible, indicating a lack of significant ongoing star formation. Minor irregularities or disturbances in the outer regions may suggest past interactions or mergers, though the dominant impression is that of a relaxed, spheroidal system.
