The galaxy presents as an elliptical or lenticular system, displaying a smooth, largely featureless morphology. The light distribution suggests a high degree of central concentration, with a gradual falloff in intensity towards the outer edges. The color gradient indicates a population of older stars dominating the galaxy's stellar content, with a notable absence of prominent blue star-forming regions. Faint hints of greenish color on the edges suggest the presence of ionized gas and some minor star formation activity, but overall the galaxy appears quiescent in terms of star formation. The shape is generally rounded, with only a slight elongation, implying a minimal rotational component. There is no obvious evidence of tidal features or interaction with neighboring galaxies. The overall impression is that of a mature, relatively isolated galaxy that is quite massive.
