The galaxy appears as a single, relatively smooth object with a concentrated central bulge. There is some indication of a slight ellipticity in its shape, but overall it presents as quite round. A color gradient is observable, shifting from a yellowish central core outward to a slightly bluer halo region. This suggests a population of older stars in the center with the possibility of ongoing, low-level star formation in the outer regions. The galaxy does not display any prominent spiral arm structures or evidence of a major ongoing merger event. There may be minor disturbances or irregularities within the outer halo, though this requires higher resolution imaging to confirm.
