The galaxy presents as an elliptical structure, exhibiting a high degree of central concentration. The light profile appears smooth with no distinct spiral arms or bar features visible. The galaxy appears to be a single component, undisturbed system. Its overall color suggests a relatively older stellar population. The absence of significant dust lanes or prominent star-forming regions supports this assessment. There appears to be minimal evidence of ongoing star formation within the galaxy. The morphology is consistent with that of a mature elliptical galaxy.
