The galaxy presents an overall elliptical morphology. The central bulge appears to be smooth and concentrated, exhibiting a bright, yellowish hue, likely indicating an older stellar population. The disk component appears relatively faint and less structured. The galaxy does not seem to display strong spiral arm features or prominent dust lanes. It also appears to be relatively undisturbed with no clear signs of major mergers. Overall the galaxy exhibits a largely uniform color gradient suggesting a lack of ongoing major star formation within the galaxy.
