The galaxy presents a generally smooth, elliptical morphology with a concentrated central bulge. The light profile appears somewhat disturbed or potentially undergoing a minor interaction, evidenced by a slight elongation or extension of the main body. Its color exhibits a redder hue, suggesting an older stellar population and a lower rate of ongoing star formation. There is a possibility this galaxy is in the process of merging or has recently merged with another galaxy due to it's irregular morphology. Overall, it appears to be a massive galaxy at a significant redshift.
