The galaxy presents a smooth, elliptical morphology. Its light profile is centrally concentrated, with a bright, diffuse core that gradually fades into the surrounding halo. There is no apparent disk structure or spiral arm features discernible. The overall color appears to be dominated by older stellar populations, exhibiting a redder hue. There is a slight indication of blue in the outer regions of the galaxy. No significant signs of recent merger activity are immediately visible, although subtle irregularities cannot be ruled out without further analysis. The general appearance indicates a relatively evolved system with a dominant spheroid component.
