The galaxy appears as a moderately bright, concentrated object. The galaxy's overall form is elliptical, or possibly a tightly wound spiral. The light distribution appears relatively smooth and centrally concentrated, with no obvious spiral arm structures or bar features discernible. The colour suggests a population of older stars, although there is some evidence of ongoing star formation. The galaxy does not appear to be undergoing any major merging events or tidal disturbances, although there is very faint possibility of a minor disturbance. The galaxy appears somewhat isolated.
