The galaxy appears to be an elongated, disk-shaped system. It exhibits a central bulge that appears yellowish, indicative of an older stellar population. The outer regions of the disk show a bluer hue, possibly signifying the presence of younger stars and ongoing star formation. The disk component shows a slight asymmetry, with a hint of faint structure but with no apparent spiral arms. The galaxy does not exhibit any signs of a major merger or significant tidal disturbances. It leans towards being a relatively massive system. The smooth appearance suggests a galaxy with an intermediate star formation rate. The shape seems to be tending more toward a cigar shape. The disk appears not perfectly edge on, but more "in between" edge on and face on. 
