The galaxy appears to be an elliptical type, elongated in shape. It exhibits a smooth, relatively featureless morphology, with a concentration of light towards the center, gradually fading towards the edges. The color gradient shifts from yellowish-orange in the core to a more greenish hue in the outer regions. This could indicate differences in stellar populations, with older, redder stars concentrated towards the center and younger, bluer stars more prevalent in the outer parts, or differential dust obscuration. There is no evidence of spiral arms or active star formation regions readily apparent. The overall shape suggests it may be viewed at a significant angle to its plane. There is a slight asymmetry to the shape, which may indicate a past or ongoing minor interaction or merger.
