The galaxy presents as a moderately redshifted, elliptical morphology with a relatively smooth appearance. It exhibits a concentrated central bulge that appears to be primarily composed of older stellar populations, as evidenced by its reddish-yellow hue. The overall shape approximates an oblate spheroid. There is no discernible evidence of spiral arms or significant dust lanes. The galaxy does not appear to be undergoing any major mergers or tidal disruptions, though there may be some very minor disturbances. The lack of prominent blue regions suggests a relatively low rate of on-going star formation. The overall structure indicates a galaxy that is relatively mature and has likely undergone significant evolutionary processes.