This galaxy appears to be a relatively smooth, elliptical system. It exhibits a central concentration of light, suggesting a prominent nucleus or core region. The overall shape is somewhat rounded, though a slight elongation is discernible, indicating a deviation from a perfect sphere. There is a noticeable color gradient within the galaxy. The central region exhibits a reddish hue, possibly indicative of an older stellar population or dust obscuration. The outer regions show a bluer tint, suggesting the presence of younger stars or a different stellar population mix. Subtle asymmetries in the light distribution are present, which might suggest minor gravitational interactions or internal disturbances. There does not appear to be a strong presence of distinct spiral arms or a well-defined disk component. No obvious signs of a major ongoing merger are visible, though some subtle irregularities might indicate past interactions or minor disturbances.
