The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. Its core appears quite bright, exhibiting a yellow-orange hue suggestive of an older stellar population. The galaxy gradually fades into a diffuse outer envelope, lacking prominent spiral arm structures or distinct features. The overall shape is more rounded than elongated. There is no readily apparent evidence of a major ongoing merger or significant tidal disturbance; however, the galaxy's light distribution could hint at a past interaction. Given its color and morphology, the galaxy likely has a relatively low star formation rate.
