The galaxy presents a generally smooth morphology with a high degree of circularity. Its core exhibits a significantly higher luminosity and a yellowish-orange hue, likely indicating an older stellar population and a lack of ongoing star formation in that region. Fainter, somewhat diffuse extensions emanate from the central region, hinting at a possible disk structure, although the resolution is insufficient to confirm prominent spiral arms. There are no obvious signs of a major merger event, though subtle asymmetries could indicate past or ongoing minor interactions. Overall, the galaxy appears to be a relatively evolved system, transitioning away from active star formation and towards a more quiescent state.
