The galaxy appears as a centrally concentrated object with a generally smooth morphology. The light profile suggests a significant bulge component. The color is primarily yellow-orange, hinting at an older stellar population and potentially a lack of significant ongoing star formation. There is no strong evidence of spiral arms or a well-defined disk structure. There is a faint extension of light surrounding the core, possibly indicating a halo or the presence of a more diffuse outer disk. Overall, it resembles an elliptical or lenticular galaxy at a substantial redshift. There is no evident interaction or tidal features visible.
