The galaxy presents as an elliptical morphology, with a high degree of central concentration. The light profile suggests a smooth stellar distribution, with no apparent spiral arm structure or prominent dust lanes. A slight elongation is visible, indicating a deviation from perfect circularity. Color gradients are subtle; the central region exhibits a yellowish-orange hue, potentially indicative of an older stellar population, while the outer regions appear slightly bluer, suggesting the presence of some younger stars, though limited. There is no visual evidence of ongoing major merger activity or significant tidal disturbances, but some minor disturbances cannot be ruled out given the fuzziness of the image. The galaxy appears relatively isolated in the field. 
