The galaxy presents a generally elliptical morphology, appearing relatively smooth in texture, with a concentrated central bulge. There's a suggestion of a faint, diffuse disk component extending outwards from the core. The color gradient transitions from a yellowish-white core to a slightly bluer, more diffuse outer region, indicating potential variations in stellar populations and age across the galaxy. There may be some minor disturbances, but there is no single dominant feature to suggest an active or recent merger event. Overall, the galaxy exhibits characteristics suggestive of an early-type spiral galaxy.
