The galaxy appears as a single, relatively smooth structure, with a moderate degree of ellipticity. Its overall color is consistent with an older stellar population and a lack of significant ongoing star formation, with a redder hue dominant throughout its morphology. There is a subtle color gradient apparent, slightly bluer towards the center, which could be from a small amount of central star formation. It is not possible to identify any distinct spiral arm structures or prominent dust lanes from the image. No clear signs of interaction or tidal disturbances are observed, based on its relatively undisturbed morphology. The galaxy does not appear to be undergoing a major merging event, although minor disturbances cannot be ruled out.
