The galaxy appears to be a relatively smooth, centrally concentrated object with a slight elongation. The dominant color is reddish-orange, suggesting an older stellar population with relatively low levels of on-going star formation. The galaxy exhibits a weak disk-like morphology. No significant spiral arm structure or dust lanes are apparent. There may be a tidal tail extending from the main body to the upper-right. There is a possible minor disturbance in the structure, but it could be a minor merger.
