The galaxy presents as a slightly elongated, lenticular-like structure. A prominent, bright central bulge is visible, exhibiting a yellowish-white hue. This likely indicates a population of older stars. Diffuse disk features extend outward from the central bulge, though with a relatively smooth texture. There is a notable lack of distinct spiral arms. The colour gradient from the center outwards suggests a decrease in stellar density, and likely a lower star formation rate in the outer regions. Overall, the galaxy appears to be an evolved system, possibly undergoing a transition from spiral to elliptical morphology.