The galaxy presents as a disc galaxy, seen edge-on. There is a pronounced central bulge, unresolved in this image, which appears to be surrounded by a bright, extended halo. The disc appears to be relatively thin, showing evidence of dust lanes along the equatorial plane, which are not well-defined. There is a hint of possible minor tidal disturbance or interaction, but more data is needed to confirm whether the distortion is due to interaction with another galaxy. The galaxy exhibits signs of ongoing star formation, evidenced by the presence of bluer regions within the disc. The galaxy is not perfectly smooth and shows some irregularities and possible spiral structures. It is cigar shaped rather than being perfectly round.