This galaxy appears to be a relatively smooth, elliptical galaxy. It is characterized by a centrally concentrated luminosity profile, suggesting an older stellar population. The galaxy exhibits an overall blueish hue, potentially indicating ongoing, though relatively low levels, of star formation within the galaxy. It is mostly symmetrical in shape, and not particularly round, perhaps slightly elongated. There seems to be some minor disturbance, possibly an interaction, that is affecting the shape, but it is likely not undergoing a major merger.