The galaxy presents as a smooth, elongated structure with a distinct central bulge. The light profile appears relatively uniform, lacking prominent spiral arms or distinct knots of star formation. The overall color suggests a population of older stars, with a central region exhibiting a more yellow or orange hue, potentially indicative of a higher concentration of evolved stellar populations. The outer regions appear slightly bluer, possibly due to the presence of some younger stars, though not significantly prominent. The galaxy exhibits a cigar shape. There is no visible evidence of a major ongoing merger or significant tidal disturbances affecting the galaxy's morphology. It appears as a relatively undisturbed system, though potential minor interactions cannot be ruled out based solely on this image.
