This galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a roughly circular morphology, with a gradual decrease in luminosity from the core outwards. The central region appears to be dominated by older stellar populations, indicated by the yellowish hue. Moving outward from the center, the color transitions to a bluer tone, suggesting a younger stellar population may be present in the outer regions, and a low level of on-going star formation may exist in the galaxy. The galaxy does not exhibit any distinct spiral arm structures or a prominent disk component. There is no apparent sign of a major ongoing merger or strong tidal interaction. The light distribution is fairly uniform, indicating a high degree of symmetry. Small-scale irregularities can be detected, possibly hinting at minor disturbances.
