The galaxy presents an overall elliptical morphology, displaying a smooth, relatively featureless light distribution.  There is a notable concentration of light towards the center, but it seems diffuse rather than a sharply defined core.  The galaxy exhibits a subtle color gradient, shifting from a bluer hue on the apparent left side to a slightly redder hue on the right. This may indicate differential stellar populations or dust content within the galaxy.  Hints of tidal disturbances or interactions are visible, in the form of faint extensions or asymmetries.  The primary body of the galaxy does appear somewhat round overall.
