The galaxy appears as a centrally concentrated, elliptical-like structure. The light distribution suggests a smooth and relatively featureless morphology. The galaxy exhibits a slight elongation, appearing more cigar-shaped than perfectly circular. A subtle color gradient is observed, with the central region appearing slightly brighter. The outer regions exhibit a bluer hue, potentially indicative of younger stellar populations. There is no apparent significant tidal disturbance or merger activity observed in the immediate vicinity.
