The galaxy presents as an elongated, cigar-shaped structure, suggesting a likely classification as an elliptical or lenticular galaxy. Its overall light distribution appears relatively smooth with a somewhat brighter central region, possibly a galactic bulge or an active galactic nucleus. The galaxy exhibits a dominant blue-white hue, which could indicate a younger stellar population or recent star formation, although given the smooth morphology, an older population is also a possibility. There is a subtle hint of some disruption in the galaxy's structure with a very slight asymmetry observed in the outer regions. This could be evidence of a past minor merger event. There are no discernible spiral arms or dust lanes visible.
