The galaxy presents as a relatively smooth, elongated structure, suggestive of a disk galaxy viewed at a high inclination angle. A central bulge is faintly discernible, appearing somewhat brighter and more concentrated than the surrounding disk. The color profile indicates a slightly bluer hue. The overall morphology leans towards a cigar-shaped profile. There's no strong indication of prominent spiral arms or active star formation regions within the galaxy. There's little sign of any major disturbances or recent merger events in the galaxy's structure.
