The galaxy presents as a centrally concentrated object, with a smooth, relatively featureless morphology. The light profile appears spheroidal, tending towards a more rounded, rather than elongated, shape. There is no strong evidence of spiral arm structures or a well-defined disk. The galaxy exhibits a color gradient, with a yellowish-orange hue dominating the core region, suggesting an older stellar population. Moving outwards from the core, the color shifts to a slightly bluer tint, possibly indicating the presence of some younger stars or ongoing star formation at a low rate. There are no indications of tidal tails, bridges, or other signs of a recent major merger event. Minor disturbances cannot be ruled out based on the image alone.
