The galaxy appears as a relatively smooth, elliptical-like structure. Its morphology is dominated by a bulge. There's a slight hint of a disk with very faint spiral arm structures. The light distribution is concentrated toward the center, indicating a high degree of central density. The galaxy exhibits a redder color, suggesting an older stellar population and low current star formation. There are no signs of significant ongoing mergers or major disturbances in the overall shape, although a subtle asymmetry may hint at a minor interaction in its past.
