This galaxy exhibits a primarily smooth, elliptical morphology. Its shape is more akin to an ellipse that is trending toward round rather than elongated, with an aspect ratio that suggests a classification between E3 and E5 on the Hubble sequence. The central region displays a concentrated luminosity, hinting at a prominent galactic bulge. The galaxy exhibits a color gradient, appearing more yellow and old toward the center. A blueish halo encompasses the core, which may indicate pockets of younger stellar populations or regions of ongoing, but slow, star formation. There is no prominent spiral arm structure visible, and there is no evidence of any significant tidal distortions. This suggests that if the galaxy has undergone any merging activity, it has been either very minor or that any such activity has occurred far in the past, as there are no major disturbances.
