The galaxy presents an elliptical morphology, appearing largely smooth and spheroidal in shape with minimal discernible substructure. The light distribution is highly concentrated towards the center. There are no clear spiral arms, bars, or obvious dust lanes visible. The color profile exhibits a generally redder hue. This suggests a stellar population dominated by older, cooler stars. The redder color could also be due to redshift. Star formation activity appears to be relatively low. The galaxy is a member of the "red sequence" of galaxies, meaning that it is a relatively massive galaxy that is no longer forming many new stars. Based on morphology, this appears to be an elliptical galaxy. There are no signs of any interactions or mergers.
