The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge with a yellowish hue, suggesting an older stellar population. The light intensity decreases gradually from the center outwards, forming a diffuse halo. There is no apparent spiral arm structure or dust lane visible in this image. The overall shape is approximately elliptical, with a slight deviation from perfect circularity. The galaxy does not display any obvious signs of ongoing major merger activity or tidal disturbances. Its color suggests a low star-formation rate.
