This galaxy presents a predominantly smooth morphology, with a slight apparent elongation. Its color profile suggests an older stellar population, primarily emitting in the redder wavelengths, although there is evidence of some bluer emission in the central regions, indicating recent or ongoing star formation. The galaxy lacks any immediately obvious spiral arm structure or significant dust lanes. It appears to be relatively undisturbed, showing no signs of a major merger event or tidal distortions. Based on its apparent shape, it is most likely an elliptical galaxy or a lenticular galaxy seen face-on. There is a slight asymmetry with the shape that could indicate a minor merger event or tidal interaction, but the galaxy generally appears relaxed.
