The galaxy presents a generally elliptical morphology, displaying a smooth, concentrated light profile. There is a lack of discernible spiral arm structures. The core exhibits a bright, yellowish-white hue, suggesting an older stellar population dominating the central regions. The galaxy shows a moderate redshift, indicating that it is relatively distant. There are no obvious signs of recent major merger activity or tidal disturbances, although minor disturbances cannot be ruled out due to the image resolution. The galaxy appears to have a small amount of ongoing star formation, given the colors and shape. The object is relatively round.
