The galaxy appears to be an elliptical galaxy. It exhibits a smooth, centrally concentrated light profile with a high degree of central brightness. The isophotes are generally round to slightly elliptical in shape. There is no evidence of prominent spiral arms, a disk, or significant dust lanes. The color profile suggests a population of older stars, with a redder hue overall. There are no obvious signs of a recent major merger or significant tidal disturbances in the immediate vicinity. The object has a well-defined core, with a smooth and regular decrease in luminosity towards its outer regions. Based on the available data, there is no indication of ongoing active star formation within the galaxy.
