The galaxy appears to be a relatively smooth, elliptical-type galaxy, seen nearly edge-on. A bright, concentrated central bulge is visible, dominating the galaxy's overall luminosity. The outer regions display a gradual fading of light intensity, with no distinct spiral arms or dust lanes discernible in the image. There are no obvious signs of ongoing major mergers or significant tidal disturbances, although minor disturbances cannot be ruled out at this resolution. The galaxy possesses a moderate red-shift, indicating it is at a significant cosmological distance. Given the apparent magnitude and distance, this galaxy is moderately luminous.
