The galaxy presents as a relatively smooth, centrally concentrated object with a somewhat elliptical morphology. Its core exhibits a bright, yellowish-white luminosity, suggesting a high density of older stellar populations or possible AGN activity. The light gradually diffuses outwards from the core into a broader, less intense halo. Hints of bluer hues in the outer regions suggests the presence of younger stars or ongoing star formation. There's a slight disturbance in the overall circularity which could indicate minor tidal interactions.
