The galaxy presents as a smooth, elliptical morphology, with a dominant central bulge. The galaxy appears relatively featureless, lacking prominent spiral arms or distinct dust lanes. The color profile suggests a predominantly older stellar population, with a redder hue. This redder hue is consistent with the observed redshift, indicating significant distance. The galaxy appears to be isolated, with no immediate signs of tidal interaction or ongoing merging events. There is a slight elongation in its shape; while it tends toward round, it is not perfectly so. Star formation is not evidently high in the galaxy's core.