The galaxy presents a generally smooth, elliptical morphology with a high degree of central concentration. The galaxy exhibits a rounded shape with no discernible disk structure or spiral arms. There is a lack of prominent dust lanes or regions of active star formation visible within the galaxy's structure. The overall color appears relatively uniform and redder, suggesting an older stellar population and low ongoing star formation activity. There is no indication of a major merger event and there does not appear to be a strong interaction with any other nearby galaxies. There may be evidence of a minor disturbance to its overall form, which is inconclusive based on the image quality.
