The galaxy appears as a relatively smooth, elliptical structure with a high degree of central concentration. The color gradient suggests a population of older stars dominating the central bulge, appearing more yellow/orange. The outer regions exhibit a slight bluish tint, hinting at the presence of a younger, though subdued, stellar population or perhaps ongoing, but modest, star formation. The overall morphology is generally featureless, with no obvious spiral arms or bar structures visible. The shape is not perfectly spherical; it shows a slight elongation, leaning more towards an in-between or mildly cigar-shaped profile rather than a perfectly round form. There's no visually striking evidence of a major merger or significant tidal disturbances, although some subtle asymmetry could indicate minor past interactions or internal dynamic processes. The galaxy's overall appearance implies a relatively evolved system with a significant fraction of its stellar mass already formed.
