The galaxy presents as a relatively smooth, amorphous structure, though there appears to be at least two concentrations of light within the main body. It is slightly elongated, with an overall color profile that is redder than it is blue, indicating a possible lack of significant ongoing star formation. There is evidence of potential tidal interactions, with what may be disturbed material surrounding the central body of the galaxy, possibly the result of a merger event. The light distribution is more concentrated centrally. Overall, this galaxy appears to be on the more massive side.