The galaxy appears as a centrally concentrated elliptical system. Its morphology is generally smooth, with a notable lack of prominent spiral arms or distinct features. The core exhibits a high surface brightness, suggesting a dense stellar population and possible presence of an active galactic nucleus (AGN). The overall shape is elongated, resembling a flattened spheroid, with a slight indication of a disk. There are hints of possible tidal distortions or minor disturbances suggesting minor gravitational interaction with a small nearby object or a past merger event. The galaxy displays a bluish hue in its outer regions, indicative of younger star formation.
