The galaxy presents a moderately elliptical morphology. Its color profile suggests a population of evolved stars, exhibiting a yellowish-white hue in the central region, with a slight bluer tint in the surrounding area, which may indicate ongoing star formation. The galaxy appears relatively undisturbed, lacking any obvious tidal features or signs of a recent major merger. There are no apparent spiral arm structures, but the outskirts exhibit a fuzzy texture which is consistent with the presense of a bulge, or diffuse halo of stars. The galaxy's size, compared to the visible field, suggests it is a distant object, likely located at a significant cosmological redshift.
