The galaxy appears to be a relatively smooth, elliptical-type galaxy. It presents with a generally rounded morphology, with an absence of defined spiral arms or a prominent disk structure. The light distribution suggests a concentration of older stellar populations. There is a slight asymmetry in the shape, potentially indicating minor gravitational disturbance or interaction with another galaxy, although no major merger features are readily apparent. The color profile leans towards the redder end of the spectrum, which supports the assertion of an older stellar population and minimal ongoing star formation activity. The small angular size, coupled with its redshift, suggests a considerable distance. 
