The galaxy presents as a moderately bright, elongated structure. Its light profile appears relatively smooth, suggesting a later-type morphology, potentially a spiral galaxy viewed at an oblique angle, or possibly a lenticular galaxy. There is a subtle suggestion of a central bulge, slightly brighter than the surrounding disc. The colour indices indicate a redder population, likely indicative of older stars and a moderate amount of dust obscuration. There may be some disturbance to the galaxy's shape, possibly a faint tidal tail or asymmetry, hinting at a past or ongoing interaction. However, this could also be due to the angle of observation. The size suggests that it is not a dwarf galaxy and likely hosts a substantial stellar mass. The star formation rate is at least modestly active.
