This galaxy appears to be an elliptical type, exhibiting a smooth, centrally concentrated light profile. There is no evidence of spiral arms or a distinct disk structure. The galaxy presents as a round shape with no major morphological disturbances suggesting recent or ongoing major mergers, though minor disturbances are possible. The core is a bright yellow-white, indicating an older stellar population. Given the redshift of the galaxy, it is at a considerable distance, explaining the lack of finer details.