The galaxy presents as a centrally concentrated object with a largely smooth morphology. The central bulge exhibits a yellowish-white hue, suggesting an older stellar population. Surrounding the bulge, a fainter, more diffuse disk is apparent. There is a slight bluing of the outer regions of the disk, possibly indicating the presence of younger stars and ongoing star formation. There is evidence of some disturbed morphology in the disk, perhaps indicating a minor interaction or merger in its past. Overall, the galaxy appears relatively isolated and well-formed.
