The galaxy presents as a slightly elongated, centrally concentrated object. A bright, yellowish core gradually diffuses outward into a larger, fainter disk. The color gradient suggests a mix of stellar populations, with the core potentially dominated by older, redder stars. Subtle hints of bluer regions can be discerned in the outer disk, possibly indicating areas of more recent star formation. Overall, the galaxy appears relatively smooth in texture, with no immediately obvious spiral arm structures or major disturbances. The morphology suggests a galaxy transitioning between a lenticular and spiral type.
