The galaxy presents a generally smooth, elliptical morphology, although some subtle features suggest a possible disk component. The central region exhibits a concentrated, bright, and yellowish color, likely indicative of an older stellar population. Moving outwards from the core, the galaxy gradually fades, with a bluer hue in the outer regions, suggesting a younger stellar population and ongoing star formation. The shape is mostly round. There is no sign of a major ongoing merger, although there are subtle disturbances possibly from a minor disturbance event. Overall, the galaxy appears relatively undisturbed.
