The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that is bright and appears to be composed of older stellar populations, indicated by the yellowish-orange hue. There is a subtle transition in color towards the outer regions of the galaxy, with the halo appearing slightly bluer, suggestive of a younger, less dominant stellar population and/or ongoing, albeit minimal, star formation. No prominent spiral arms or distinct dust lanes are visible. The galaxy does not show signs of significant tidal disturbances or interactions, suggesting relative isolation and gravitational stability.
