The galaxy presents an overall elliptical morphology, exhibiting a smooth and diffuse light profile. The central region displays a higher concentration of light, appearing brighter and more yellowish in color, possibly indicating an older stellar population. Fainter, bluer extensions are observed on the periphery, suggesting the presence of younger stars or regions of ongoing star formation. No distinct spiral arms or bar structures are discernible. There is a small secondary object in close proximity to the galaxy, which appears to be undergoing a minor interaction. Overall, the galaxy exhibits a moderate redshift, implying that it is a very large and old galaxy. The galaxy appears to be undergoing only very minor interaction if any. 
