The galaxy presents as an elongated, cigar-shaped structure, likely a spiral galaxy viewed at a high inclination. The central region exhibits a concentrated luminosity, suggestive of a galactic bulge. The disk appears relatively smooth, with a hint of bluer hues along the edges, possibly indicating areas of more recent star formation within the spiral arms. There may be some slight disturbances in the outer disk, but there is no strong evidence of a major ongoing merger.
