The galaxy presents a relatively smooth appearance with a possible very faint, diffuse disk. The overall shape tends towards being in between round and elliptical, with a slight elongation noticeable. There is no strong evidence of spiral arm structure or a distinct central bulge. The light distribution appears centrally concentrated, fading outwards to the edges of the galaxy. The galaxy color appears moderately blue, suggesting the presence of some younger stellar populations and potential recent star formation, although the smoothness suggests that this may be limited. There is no obvious evidence of a major ongoing merger event or significant tidal disturbances, though some slight asymmetry cannot be ruled out. The general morphology suggests that this is a relatively evolved galaxy, possibly a lenticular or early-type spiral.
