The galaxy appears to be a relatively smooth, elliptical galaxy at redshift z ≈ 0.109. It exhibits a yellow-orange hue, suggesting a population dominated by older stars. The galaxy displays an overall elongated shape, with the major axis being significantly longer than the minor axis. There is a slight distortion of the smooth profile on one side of the galaxy. There is little evidence of spiral arms or prominent dust lanes. Star formation rates are estimated to be very low. The galaxy appears to be relatively isolated, with no obvious signs of ongoing major merger activity.
