The galaxy appears as a centrally concentrated, relatively smooth object with an elliptical morphology. The light distribution suggests a dominant bulge component, with a lack of discernible spiral arm structure. The color is generally consistent across the galaxy, with a slight redder hue, implying an older stellar population with relatively low ongoing star formation. There is no sign of tidal features, strong dust lanes, or morphological peculiarities indicative of a recent major merger, though minor disturbances cannot be ruled out at this resolution. The galaxy appears fairly isolated in the field.
