The galaxy presents a predominantly smooth morphology, lacking strong spiral arm features or a distinct bar. It appears elliptical in shape, with a noticeable elongation. The central region exhibits the highest surface brightness, suggesting a concentrated nucleus or bulge. The overall color profile indicates a population of older stars, contributing to a yellowish-white hue. The outer regions show a gradual decrease in luminosity, fading into the background sky. There is no indication of any significant recent merging activity or major disturbances in its structure. Subtle variations in color across the galaxy might suggest regions of varying stellar populations.
