The galaxy presents as an elliptical morphology, exhibiting a smooth, diffuse light profile with no readily discernible spiral arm structure or prominent dust lanes. The central region appears slightly brighter than the outer regions, indicative of a concentrated nucleus. The galaxy appears moderately rounded. There is no strong evidence of tidal tails or significant morphological distortions, suggesting it is relatively undisturbed and not undergoing a major merger event, although there may be some minor disturbances. The galaxy displays a yellowish-white color, suggesting an older stellar population with relatively low ongoing star formation. The galaxy appears to have a small angular size on the sky, implying a moderate physical size. The redshift suggests this is a relatively distant object.