The galaxy presents an elliptical morphology, appearing elongated with a high degree of axial ratio. Its light distribution is smooth and centrally concentrated, indicative of an older stellar population. The primary color is a warm yellow-orange hue, suggesting a dominance of evolved stars with lower rates of recent star formation. There is no discernible evidence of spiral arms, dust lanes, or prominent star-forming regions. The galaxy does not show signs of any major ongoing merger activity, although minor disturbances cannot be ruled out due to the resolution limitations. Overall, it appears to be a relatively quiescent and massive galaxy.
