The galaxy presents as a concentrated, elliptical object, approximately 10 kpc in radius. The morphology appears largely smooth, with a dominant central bulge exhibiting a yellowish-orange hue, suggesting an older stellar population. A faint, diffuse halo surrounds the central region, fading gradually into the background. There is no obvious spiral structure or disk component visible in this image. The overall structure indicates minimal signs of ongoing mergers or major disturbances. The galaxy is largely spheroidal in shape, not significantly elongated.
