The galaxy appears as a roughly elliptical object with a smooth, diffuse light distribution. A bright central region dominates the visual appearance, suggesting a higher concentration of stellar density and potentially an active galactic nucleus. There is a noticeable color gradient, with the central region exhibiting a yellow-white hue, which possibly indicates an older stellar population. The outer regions appear slightly bluer, which could signify the presence of younger, hotter stars, or ongoing star formation. The galaxy exhibits no obvious spiral arm structures or dust lanes, lending support to its classification as elliptical. There are slight hints of asymmetry in the outer regions, possibly indicating a past minor merger event or gravitational interaction, though the disturbance is not significant. Overall, the galaxy presents itself as a massive, evolved system undergoing relatively low levels of star formation.
