The observed galaxy presents a disturbed morphology, suggestive of an ongoing or recent merger event. There appear to be two distinct nuclei or high-density regions of stars within the galaxy's central region, indicating a potential interaction between two separate galaxies. The shape of the galaxy is elongated and asymmetrical, diverging from a regular elliptical or spiral form. A significant portion of the galaxy's light emanates from a relatively compact area, suggesting a high concentration of stars and possibly active star formation in that region. The galaxy exhibits a redder color, which could be indicative of an older stellar population, dust obscuration, or the effects of redshift due to its distance. There are no clearly defined spiral arms or a prominent disk structure visible.
