The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a noticeable central bulge, which appears brighter and more concentrated than the outer regions. The color profile suggests a population of older stars, evident in the yellowish-white hue, particularly prominent in the central bulge. There is a hint of a disk-like structure, although it is not clearly defined and appears somewhat irregular. The outer regions of the galaxy fade gradually, lacking sharp boundaries. There's minimal evidence of ongoing star formation or prominent spiral arms. Based on the moderate red shift, the galaxy is at a considerable distance, which, combined with the morphological data, suggests that it could be an intermediate mass galaxy that could be undergoing some minor disturbance. There does not seem to be any major mergers or artifacts.