The galaxy presents as a somewhat smooth, centrally concentrated object, with a general elliptical morphology. There is evidence of tidal interactions, and a likely merger event as the galaxy appears to have two distinct nuclei. The galaxy exhibits a yellow-red hue, suggesting an older stellar population and a relatively low rate of star formation. Faint disturbed structures or tidal tails are present, supporting the merger hypothesis. The light distribution is primarily centrally concentrated.
