This galaxy appears to be a relatively smooth, elliptical galaxy, likely at an intermediate redshift. It presents as a concentrated central bulge of older stars exhibiting a yellowish-orange hue, indicative of an evolved stellar population. The overall light distribution is generally smooth, lacking prominent spiral arms or distinct features. The galaxy exhibits a slightly rounded shape, with no obvious signs of significant tidal disturbances or recent major merger events. However, there may be a close companion in the process of merging with the main galaxy. The overall color suggests a relatively low ongoing star formation rate.
