The galaxy in question appears as a relatively compact object with a moderate level of overall surface brightness. There is some indication of a possible disturbance in the overall morphology, but the evidence is subtle. The galaxy does not appear to have a classic spiral structure. There is a possible hint of a tidal tail or a bridge feature, but is indistinct. Some asymmetry in the light distribution hints at a possible interaction or merging event. There may be a faint extended halo surrounding the central region, but the faintness makes it difficult to confirm. The colours appear consistent with a relatively old stellar population.
