The galaxy presents as a centrally concentrated object with a relatively smooth, diffuse morphology. The core exhibits a bright, yellowish-white luminosity, indicative of a significant stellar population density and/or the presence of an active galactic nucleus (AGN), although the image resolution limits conclusive determination. Fainter, less structured, and bluer regions are observed extending from the central region of the galaxy. Overall, the galaxy does not display pronounced spiral arms or strong dust lanes, suggesting it may be an elliptical galaxy. There is little evidence of recent major merger events.
