The galaxy appears to be a relatively smooth, elliptical type. It exhibits a dominant central bulge, with a less defined disk component. The color profile suggests an older stellar population, with a redder hue throughout the galaxy indicating a lack of significant ongoing star formation. The shape is somewhat elongated, but not drastically so, appearing more "in between" round and cigar shaped. There are no obvious signs of recent major mergers or significant tidal disturbances.