The galaxy appears to be a relatively smooth, elliptical galaxy with a centrally concentrated light profile. The core exhibits a bright, yellowish hue, suggesting an older stellar population. Moving outwards from the core, the light gradually fades, maintaining a generally elliptical shape. There is no prominent evidence of spiral arms or a well-defined disk structure. The galaxy appears mostly undisturbed with no major asymmetries or tidal features visible, suggesting it has not undergone a major merger recently. The galaxy exhibits a moderate redshift, indicating it is at a substantial cosmological distance.
