The galaxy presents an overall elliptical morphology, with a smooth, centrally concentrated bulge. The light distribution suggests a relatively evolved stellar population, particularly in the central region, exhibiting a yellowish-orange hue. Some disk features may be present. There is evidence of recent star formation. There are no obvious signs of ongoing major mergers, although some minor asymmetries or tidal features cannot be ruled out based on the image alone. The galaxy does not appear to be highly inclined along our line of sight.
