The galaxy appears as a roughly circular, relatively smooth object. Its color suggests a relatively older stellar population, primarily emitting in the redder bands, with a hint of bluer emission concentrated toward the galaxy's central region. There is some indication of a disk-like structure, though the overall morphology leans toward a more spheroid shape. There are no major disturbances in the image. There are no signs of a major merger, though there is some subtle asymmetry in the outer regions which may indicate a minor interaction or internal disturbance. The galaxy does not display strong evidence of active star formation across its entirety, possibly just the core. The light is diffuse, suggesting that it is an older galaxy, likely less massive, and possibly with lower star formation rates.
