The galaxy presents a somewhat elongated, cigar-like morphology. It appears largely smooth in structure, though there may be some very faint hints of a disk or other subtle features. There is no obvious evidence of spiral arms or a distinct central bulge, leading to a classification towards the elliptical end of the Hubble sequence. No strong signs of recent or ongoing major mergers. However, subtle asymmetries exist within the galaxys profile which could be due to a minor disturbance event, such as tidal interactions with a nearby satellite galaxy or another past gravitational interaction. The color profile is generally consistent throughout the galaxy's structure.
