The galaxy appears to be a spiral, viewed at a moderate angle that is neither face-on nor edge-on. There is a central bulge that is bright and concentrated, with a smooth appearance. The spiral arms are somewhat flocculent and asymmetrical, suggesting a disturbed morphology. These arms exhibit a mix of blue and red colors, likely indicating a combination of ongoing star formation and older stellar populations. The galaxy does not exhibit a highly defined spiral structure, and some tidal features or signs of interaction may be present, possibly a minor disturbance. Overall shape suggests a transitional morphology between elliptical and spiral. The outer regions of the galaxy are fainter and more diffuse than the central region.
