The galaxy appears to be a relatively smooth, elongated elliptical. The central bulge is prominent and exhibits a slightly reddish hue, suggestive of an older stellar population. There is a subtle disk component visible, although it is not sharply defined. Overall, there isn't an abundance of distinct features in the galaxy's structure; it seems to lack prominent spiral arms or significant dust lanes. The general form is cigar-shaped. There is no obvious indication of a recent major merger or strong tidal disturbances. 
