The galaxy appears as a relatively smooth and rounded object. There is little evidence of spiral arm structure or significant irregularities in its morphology. The overall color suggests a dominant population of older stars, implying a relatively low star formation rate. A hint of bluer colors in a few localized regions may indicate the presence of younger stellar populations, albeit not widespread. There appears to be little to no tidal disturbance, indicating that it has not undergone a recent major merger event. It shows only a minor asymmetry.