The galaxy presents a largely smooth and elliptical morphology, with a high degree of central concentration. The light profile appears centrally bright and gradually fades towards the outer edges. The galaxy exhibits a yellowish hue indicative of an older stellar population. There is minimal evidence of spiral arm structure, nor are any significant dust lanes visible. Faint, subtle irregularities in the outer regions are possibly present, suggesting some minor gravitational interaction. Overall, the galaxy shows a lack of ongoing star formation with a dominant population of evolved stars.
