The galaxy presents as a relatively smooth, centrally concentrated object. It appears elliptical in shape, with a high degree of roundness. The galaxy exhibits a dominant yellowish-orange hue, suggesting an older stellar population. There is little evidence of spiral arm structure or significant dust lanes. No clear signs of ongoing major merging events are observed; however, a slight asymmetry or minor disturbance cannot be entirely ruled out. The light profile appears smooth and gradually fades towards the edges. The size is small, suggesting that it is either an intrinsically compact galaxy or relatively distant. The red color suggests this could also be a red and dead galaxy.
