The galaxy appears to be an elliptical type, exhibiting a generally smooth and centralized light distribution. The core region presents a yellowish-orange hue, suggesting an older stellar population. The galaxy shows an elongated shape, deviating somewhat from perfect circularity. There are hints of faint, diffuse outer regions extending from the main body, appearing slightly bluer in color, indicative of some ongoing or recent star formation, although at a low rate. There are no significant signs of strong tidal features, major disturbances, or a recent merger event; the structure seems relatively relaxed.
