The galaxy presents as an elliptical or lenticular type system. It exhibits a generally smooth and symmetrical morphology, with a high degree of central concentration. The core region is bright and appears reddish-yellow, suggesting an older stellar population. Progressing outward from the core, the light intensity gradually diminishes. There is minimal evidence of spiral arms or significant dust lanes. Faint blue emissions surround the main body suggesting some small degree of star formation is present. No major interaction or merging events are apparent. Overall the morphology suggests a relatively evolved system.
