The galaxy presents as a largely featureless, smooth object with a generally elliptical morphology, appearing nearly circular. A concentration of light is observed toward the central region of the galaxy, gradually decreasing in intensity toward the outer edges. The color gradient indicates a dominant population of older stars in the central bulge, with a slight bluer hue in the outer regions, possibly suggesting some ongoing, albeit limited, star formation. There is no discernible spiral arm structure, nor is there evidence of significant tidal disturbances or mergers. Overall, the morphology suggests a relatively undisturbed system.
