The galaxy presents a somewhat elongated, cigar-shaped morphology. A substantial portion of its light appears relatively smooth and featureless, yet with a presence of internal structure. There is evidence of possible disruption in the form of a faint tidal tail extending outwards, indicative of past gravitational interaction. The galaxy core exhibits a moderate concentration of light, with colors skewing towards the redder end of the spectrum. Patches of bluer emission are present, possibly regions of ongoing star formation. There is an indication of a minor disturbance in the form of some irregular emission within the galaxy.
