The galaxy presents a largely smooth and featureless morphology, with a somewhat elliptical appearance. The overall color profile leans towards redder wavelengths, suggesting an older stellar population and potentially ongoing or recent star formation. There is a slight elongation, but it does not appear highly flattened, instead displaying a more spheroidal structure. No prominent spiral arms or bar structures are discernible. Subtle variations in color and intensity are present, hinting at possible substructure or internal dust lanes. The galaxy does not appear to be undergoing any major merger activity, but subtle disturbances could be present. The edges appear to be smooth, without a lot of distortion. Overall, the galaxy gives the appearance of being in a relatively relaxed state, with a high degree of symmetry.
